STARBURST GALAXIES:
NEAR AND FAR
Ringberg Castle, Germany
10 - 15 September 2000
email: ringberg@mpe.mpg.de
URL:
http://www.mpe.mpg.de/www_ir/ringburst2000.html
Further information will be posted and regularly updated on this website.
31 Mar 2000 | Deadline for abstract submissions |
THE DEADLINE HAS PASSED. NO MORE ABSTRACTS WILL BE ACCEPTED. | |
1 May 2000 | Acceptance Notification and Second announcement |
Summer | Final announcement |
10 Sep 2000 | Arrival at Ringberg |
11-15 Sep 2000 | Scientific Sessions |
15 Sep 2000 | Departure from Ringberg at 18:00 (Hotels in Munich for Friday 15 to Saturday 16) |
This marks the end of the First Announcement. Click here to go back to the top of the page.
F. Bertoldi | Invited Highlight | Results from MAMBO mm Surveys |
C. Carilli | Invited Highlight | Deep Radio Surveys of Star Forming Galaxies |
C. Cesarsky | Invited Review | ISOCAM Survey Results |
S. Charlot | Invited Review | Modeling Stellar Populations at Low and High z |
F. Eisenhauer | Invited Highlight | The Low Mass End of the IMF in Clusters |
N. Foerster-Schreiber | Invited Highlight | ISO Evidence of Star Forming Histories in Dusty Starbursts |
A. Franceschini | Invited Review | Cosmic Star Forming History: The Need for IR Observations |
U. Fritze-von Alvensleben | Invited Highlight | The Role of Chemical Evolution in Starburst Galaxies |
G. Gilmore | Invited Review | Evidence in Favor of a Universal IMF |
J. Graham | Invited Highlight | TBD |
G. Hasinger | Invited Review | Cosmic Star Forming History: The Need for X-ray Observations |
T. Heckman | Invited Review | Starbursts Near and Far: An Overview |
R. Ivison | Invited Highlight | Results from SCUBA submm Surveys |
G. Kauffmann | Invited Review | Formation of Bulges and Ellipticals: Later through Mergers |
D. Kunth | Invited Highlight | Starbursts in Blue Compact Dwarf Galaxies |
C. Mihos | Invited Review | Modeling Merger Induced Star Formation |
A. Moorwood | Invited Highlight | Star Forming Galaxies from z=2.2
H![]() |
C. Norman | Invited Review | Triggering and Quenching: Physical Processes |
B. Poggianti | Invited Highlight | Optical Spectra of Dusty Starbursts |
A. Renzini | Invited Review | Formation of Bulges and Ellipticals: Early through Bursts |
G. Rieke | Invited Review | Nearby Dusty Starbursts |
D. Rigopoulou | Invited Highlight | Star Formation Properties of ISOCAM Galaxies |
D. Schaerer | Invited Review | Stellar Signatures in Integrated Spectra |
A. Sternberg | Invited Review | The Interplay between ISM and Star Formation |
B. Whitmore | Invited Highlight | Star Clusters in Mergers |
L. Yan | Invited Highlight | Emission Line Galaxies from NICMOS Surveys |
This marks the end of the List of Confirmed Invited Speakers. Click here to go back to the top of the page.
at the latest. Once we have your form, we will make accommodation reservations for you.
The scientific sessions will begin on Monday, 11 September at 9 AM, and end on Friday evening, 15 September. Participants should plan to arrive in the Munich area by Sunday, 10 September or earlier. We plan to hire a bus to take participants from the Munich area to Ringberg Castle on Sunday, leaving the Munich airport and downtown Munich in the mid-afternoon. People wishing to use this bus should indicate this on the registration form. The bus will return participants to Munich on Friday 15 September, leaving Ringberg at about 6 PM. Details about bus departure times and locations will be given in the final announcement.
The final program, including complete lists of talks and posters will be sent out to all participants in mid-summer. Due to time constraints and our desire to leave sufficient time for open discussion, we have scheduled some presentations as posters, but poster presenters will have the opportunity to summarize their work in the discussion sessions throughout the workshop.
STARBURSTS NEAR AND FAR, RINGBERG 10-15 SEPTEMBER 2000 | ||||
Sunday, 10th | ||||
SESSION | TIME | LENGTH | SPEAKER | TITLE |
18:00 | ARRIVAL AND REGISTRATION | |||
19:00 | WELCOME BUFFET | |||
Monday, 11th | ||||
SESSION | TIME | LENGTH | SPEAKER | TITLE |
08:45 | 0:15 | LOC | ||
09:00 | 0:35 | Heckman (R) | Starbursts Near and Far: an Overview | |
THE IMF | 09:40 | 0:15 | Figer (C) | The Initial Mass Function in the Galactic Center |
10:00 | 0:15 | Melnick (C) | The IMF in Starbursts | |
10:20 | 0:30 | COFFEE | ||
MINI-DEBATE: Universal IMF? | 10:50 | 0:25 | Gilmore (R) | Evidence in favor of a Universal IMF |
11:15 | 0:25 | Eisenhauer (R) | Evidence in favor of IMF variations | |
11:45 | 0:45 | DISCUSSION (led by Puxley) | ||
12:30 | 1:30 | LUNCH BREAK | ||
STAR FORMATION IN DIFFERENT ENVIRONMENTS | 14:00 | 0:25 | Morris (R) | Star Formation in the Galactic Center and Nearby Nuclei |
14:30 | 0:25 | Gavazzi (R) | Star Formation in Galaxy Disks | |
15:00 | 0:15 | Colina (C) | Multifrequency studies of nuclear star formation and AGN fueling in galaxies | |
STARBURST/AGN CONNECTION | 15:15 | 0:55 | DISCUSSION (led by Veilleux) + COFFEE | |
16:10 | 0:25 | Rieke (R) | Nearby Dusty Starbursts | |
16:40 | 0:15 | Kunth (H) | Star Formation in Blue Compact Dwarf Galaxies | |
17:00 | 0:15 | Kobulnicky (C) | Signatures of the Youngest Starbursts | |
17:20 | 0:15 | van Breugel (C) | The BIGGEST Starbursts at the HIGHEST redshifts | |
HOW LUMINOUS CAN STARBURSTS BE? | 17:40 | 0:45 | DISCUSSION (led by Armus) | |
18:30 | DINNER | |||
Tuesday, 12th | ||||
SESSION | TIME | LENGTH | SPEAKER | TITLE |
08:50 | 0:10 | LOC | ||
STAR CLUSTERS | 09:00 | 0:15 | Whitmore (H) | Star Clusters in Mergers |
09:20 | 0:25 | Mengel & Gilbert (C) | Star Clusters in Mergers: VLT and Keck results | |
YOUNG STAR CLUSTERS AND GLOBULAR CLUSTERS | 09:45 | 1:00 | DISCUSSION (led by Vacca) + COFFEE | |
TRIGGERING AND QUENCHING | 10:45 | 0:25 | Norman (R) | Triggering and Quenching: Physical Processes |
11:15 | 0:25 | Mihos (R) | Modeling Merger Induced Star Formation | |
11:45 | 0:15 | Lehnert (H) | Feedback by Supernovae and Superwinds | |
12:05 | 0:15 | van der Werf (C) | The Properties of Extreme Starbursts in Merging Galaxies | |
12:30 | 1:30 | LUNCH BREAK | ||
STAR FORMATION AND THE ISM | 14:00 | 0:25 | Sternberg (R) | The Interplay between the ISM and Star Formation |
14:30 | 0:15 | Burkert (C) | The Star Formation History of Interacting Spiral Galaxies | |
14:50 | 0:15 | Solomon (C) | Starburst Mechanisms in Molecular Clouds: GMCs and ULIRGs | |
15:10 | 0:15 | Scoville (C) | Starbursting in Spiral Arms and ULIRGs | |
THE ISM-STARBURST CONNECTION | 15:25 | 1:10 | DISCUSSION (led by Harris) + COFFEE | |
DEBATE: Formation of Bulges and Ellipticals | 16:35 | 0:25 | Renzini (R) | Early: Through Bursts |
17:00 | 0:25 | Kauffmann (R) | Late: Through Mergers | |
17:25 | 1:00 | DISCUSSION (led by Aretxaga) | ||
18:30 | DINNER | |||
Wednesday, 13th | ||||
8:30 - 22:00 EXCURSION, HIKE, CONFERENCE DINNER | ||||
Thursday, 14th | ||||
SESSION | TIME | LENGTH | SPEAKER | TITLE |
GLOBAL PROPERTIES | 09:00 | 0:25 | Charlot (R) | Modeling Stellar Populations at Low and High z |
09:30 | 0:25 | Schaerer (R) | Stellar Signatures in Integrated Spectra | |
10:00 | 0:15 | Gonzales Delgado (C) | Stellar Population of Nearby Starbursts | |
10:20 | 0:40 | COFFEE | ||
11:00 | 0:15 | Förster-Schreiber (H) | Star Formation Histories of Starbursts from ISO | |
11:20 | 0:15 | Fritze-von Alvensleben (H) | Chemical Evolution in Starbursts | |
11:40 | 0:15 | Dopita (C) | Chemical Abundances and Evolution in Nearby Starbursts | |
CAN WE DATE STARBURSTS? | 11:55 | 0:35 | DISCUSSION (led by Lançon) | |
12:30 | 1:30 | LUNCH BREAK | ||
14:00 | 0:15 | Poggianti (H) | Optical Spectra of Dusty Starbursts | |
14:20 | 0:15 | Rigopoulou (H) | Star Formation Properties of ISOCAM Galaxies | |
14:40 | 0:15 | Moorwood (H) | Star forming Galaxies from z=2.2 H![]() |
|
15:00 | 0:15 | Graham (H) | TBD | |
15:20 | 0:30 | COFFEE | ||
15:50 | 0:15 | Moran (C) | Hard X-Rays from Starburts Near and Far | |
16:10 | 0:15 | Calzetti (C) | UV to FIR SEDs of Starbursts | |
16:30 | 0:15 | Thompson (C) | The distribution of Star Formation Between Starbursts and Normal Galaxies from NICMOS Observations | |
16:50 | 0:40 | POSTERS | ||
HOW TO CORRECT FOR DUST EXTINCTION | 17:30 | 1:00 | DISCUSSION (led by Meurer) | |
18:30 | DINNER | |||
Friday, 15th | ||||
SESSION | TIME | LENGTH | SPEAKER | TITLE |
COSMIC STAR FORMATION HISTORY | 09:00 | 0:25 | Cesarsky (R) | ISOCAM survey results |
09:30 | 0:15 | Yan (H) | Emission Line Galaxies from NICMOS Surveys | |
09:50 | 0:15 | Ivison (H) | Results from SCUBA Surveys | |
10:10 | 0:15 | Bertoldi (H) | Results from MAMBO Surveys | |
10:30 | 0:40 | COFFEE | ||
11:10 | 0:15 | Carilli (H) | Deep Radio Surveys | |
11:30 | 0:15 | Sanders (C) | Nature of the ISOPHOT FIR Deep Field Sources | |
CONTRIBUTION OF DIFFERENT COMPONENTS TO FIR/SUBMM BACKGROUND | 11:45 | 0:40 | DISCUSSION: (led by Dole) | |
12:30 | 1:30 | LUNCH BREAK | ||
14:00 | 0:15 | Blain (C) | The History of Starburst Galaxies | |
DEBATE: How to best explore high-z star formation | 14:20 | 0:25 | Adelberger (R) | Cosmic SF history: The UV Takes it All |
14:45 | 0:25 | Franceschini (R) | Cosmic SF history: The Need for IR Observations | |
15:10 | 0:25 | Hasinger (R) | Cosmic SF history: The Need for X-rays | |
15:35 | 1:30 | DISCUSSION (led by Genzel) + COFFEE | ||
SOC/LOC | Conference End | |||
18:00 | BUS DEPARTURE TO MUNICH |
Poster boards of size 125cm×150cm will be available at Ringberg. For those who have been assigned posters, you will have the opportunity during the discussions to present the salient points of your work. Furthermore, we welcome those participants with oral presentations to bring posters highlighting some of their results. We ask that you inform us in advance that you plan to do this to assist us in planning. Posters will remain on display for the entire duration of the workshop.
Some of the crucial topics, namely universality of the IMF, the formation of ellipticals and bulges, and ways to explore the cosmic star formation history, are addressed in the form of short debates. Each debate will be introduced by two or three introductory reviews giving to the point presentations of the complementary viewpoints, followed by an extended open discussion period.
There will be a published proceedings for the workshop. We are still negotiating the terms of publication with a few publishers, and we will have final details including information about lengths, and LaTeX macros in the final announcement.
There will be a registration fee of DM 350 (about $175 (U.S.)) for participants and DM 175 for accompanying persons which will be payable in cash (German Marks) at the meeting. This will cover costs of the opening dinner, transportation to and from Ringberg from Munich, transportation to and from the Wednesday outings, the conference dinner on Wednesday evening, a soft-cover copy of the proceedings, and conference materials. We cannot take payment by credit cards, so participants should come to Ringberg with sufficient amounts of German Marks to cover this fee. To register for the workshop, please return the registration and accommodation preference forms as soon as possible, and by June 15, 2000 at the latest.
For those participants from countries requiring a visa to enter Germany, it is best to start the application procedure several months before the workshop. Please check with your local German Consulate or travel agent for information about required travel documents.
Participants should start to plan their travel to the Munich area soon. Mid to late September is Oktoberfest season, the busiest travel time of the year in Munich. Flights and hotels are booked well in advance, especially the inexpensive ones.
By air: The Munich Franz-Josef Strauss Airport lies approximately 17 km and 30 km north-east of Garching and Munich, respectively. Most major carriers offer service to Munich, although often with stopovers involved on the more distant (North American, for example) routes. There are many cheap fares available if you shop around, and these will normally require staying over one Saturday night. Many of the best deals may not be available in the busy September travel season, however. For participants arriving in the area already on Friday or Saturday the LOC can arrange for hotel accommodations in Munich.
By train: Munich Central Station can be reached from anywhere within Europe. From there, there are good public transportation connections to all of Munich. There are even railway connections to Tegernsee, in the vicinity of Schloß Ringberg.
By car: Schloß Ringberg is located about 70 km SE of Munich. For those interested in driving directly to the castle on Sunday, 10 September the LOC can send out detailed maps and instructions in advance of the workshop. Most major car rental companies have branches at the Munich Airport. Cars usually need to be reserved in advance, and rates are often more favorable if the cars are booked by an overseas travel agent. There is ample parking at the castle, and at the hotels in Kreuth and Rottach-Egern near the castle. For those staying in Munich either before or after the workshop, note that parking can be a problem there and is often quite expensive as well.
Travel to Schloß Ringberg: We will hire a bus to take participants from the airport and Munich hotels to the workshop. This bus will leave the airport at 3 PM on Sunday, September 10, and stop to pick up the participants lodged in the two Munich hotels about 45 minutes later. The trip to Ringberg Castle will take about one and a half hours from there. For those who prefer to drive their own cars, we can provide maps in advance. The bus will return participants to central Munich on Friday evening arriving about 7:30 PM.
During the workshop, many participants will be lodged at Ringberg Castle. The castle has 34 bedrooms, 7 of which can be used as doubles. Since, at full capacity, the castle can lodge only 40 people, it will be necessary for some participants to stay in hotels in the nearby villages of Rottach-Egern and Kreuth. The cost for the 5 night stay at the Castle including all meals except Sunday and Wednesday dinner will be about DM 700 ($350 (U.S.)) per person. For participants and accompanying persons staying in hotels, it may be possible to take lunch and dinner at the castle for a cost of about DM 20 per meal. However, there is a limit of 65 people imposed by the dining room at Ringberg, so that it may not be possible to accommodate all accompanying persons for all meals. Special dietary requests are happily accommodated provided advance notice is given. If you have any requests (e.g. vegetarian meals) please indicate this on the registration form.
The room rates in the village hotels range from about DM 100 to DM 160 per night for the cheapest single and the most expensive double, respectively, including breakfast. Due to the limited recreational facilities up at Schloß Ringberg, those people traveling with accompanying persons and/or families will preferably be lodged in hotels. Daily transportation from the village hotels to the castle (about a 10-15 minute drive) will be provided by the LOC.
For the weekends immediately before and after the conference (Friday and Saturday nights), we have reserved a block of about 35 hotel rooms in Munich for those participants wanting to spend some extra time in the area, or needing to stay to get cheap flights. These rooms will be given out on a first come, first serve basis. We emphasize that most hotels in the Munich area are already sold out for the weekends before and after the conference. Room rates for these hotels range from DM 150-300 for doubles or singles. We note also that the rates are cheaper for the weekend before the conference than for the one immediately after it because of the start of Oktoberfest.
The LOC will make arrangements for lodging during the conference for all participants and their accompanying persons, as well as for the weekends before and after the conference as long as we still have available rooms. We will do our best to adhere to everyone's wishes. Unfortunately, we can't make reservations for extended side trips. We will send along your accommodation booking information and payment options as soon as we make the booking. Credit cards are now accepted at most hotels including Ringberg Castle. We will notify you if there are exceptions to this. Participants should indicate all their lodging preferences on the registration form.
Bavarian weather in the early autumn is usually pleasant with daytime highs around 20° C (68° F) and nighttime lows near 5° C (41° F). Of course, this being central Europe, one should always be prepared for rapid weather changes and rain, especially for the outing in the mountains.
Any questions or problems can be directed via e-mail to either Linda Tacconi or Dieter Lutz at the dedicated Workshop account: ringberg@.mpe.mpg.de, or fax (49-89-3299-3569).
This marks the end of the Second Announcement. Click here to go back to the top of the page.
if you have not yet received your lodging arrangements. Any further information on both scientific and logistical aspects of the meeting will be posted at: http://www.mpe.mpg.de/www_ir/ringburst2000.html
For those of you who wish to travel directly from the Airport to Tegernsee by train (rather than taking the conference bus) we offer the following schedules, as well as the compilation of all schedules (useful in case of delays):
Depart Airport | Arrive at Tegernsee |
12:46 | 14:35 |
13:46 | 15:36 |
14:46 | 16:35 |
15:46 | 17:36 |
16:46 | 18:35 |
17:46 | 19:36 |
18:46 | 20:35 |
19:46 | 21:36 |
20:46 | 22:58 |
STARBURSTS NEAR AND FAR, RINGBERG 10-15 SEPTEMBER 2000 | ||||
Sunday, 10th | ||||
SESSION | TIME | LENGTH | SPEAKER | TITLE |
18:00 | ARRIVAL AND REGISTRATION | |||
19:00 | WELCOME BUFFET | |||
Monday, 11th | ||||
SESSION | TIME | LENGTH | SPEAKER | TITLE |
08:45 | 0:15 | LOC | ||
09:00 | 0:35 | Rieke (R) | Starbursts Near and Far: an Overview | |
THE IMF | 09:40 | 0:15 | Figer (C) | The Initial Mass Function in the Galactic Center |
10:00 | 0:15 | Melnick (C) | The IMF in Starbursts | |
10:20 | 0:30 | COFFEE | ||
MINI-DEBATE: Universal IMF? | 10:50 | 0:25 | Gilmore (R) | Evidence in favor of a Universal IMF |
11:15 | 0:25 | Eisenhauer (R) | Evidence in favor of IMF variations | |
11:45 | 0:45 | DISCUSSION (led by Dopita [TBC]) | ||
12:30 | 1:30 | LUNCH BREAK | ||
STAR FORMATION IN DIFFERENT ENVIRONMENTS | 14:00 | 0:25 | Morris (R) | Star Formation in the Galactic Center and Nearby Nuclei |
14:30 | 0:25 | Gavazzi (R) | Star Formation in Galaxy Disks | |
15:00 | 0:15 | Colina (C) | Multifrequency Studies of Nuclear Star Formation and AGN Fueling | |
STARBURST/AGN CONNECTION | 15:15 | 0:55 | DISCUSSION (led by Veilleux) + COFFEE | |
16:10 | 0:25 | Rieke (R) | Nearby Dusty Starbursts | |
16:40 | 0:15 | Meurer (H) | Star Formation in Blue Compact Dwarf Galaxies | |
17:00 | 0:15 | Kobulnicky (C) | Signatures of the Youngest Starbursts | |
17:20 | 0:15 | van Breugel (C) | The BIGGEST Starbursts at the HIGHEST redshifts | |
HOW LUMINOUS CAN STARBURSTS BE? | 17:40 | 0:45 | DISCUSSION (led by Armus) | |
18:30 | DINNER | |||
Tuesday, 12th | ||||
SESSION | TIME | LENGTH | SPEAKER | TITLE |
08:50 | 0:10 | LOC | ||
STAR CLUSTERS | 09:00 | 0:15 | Whitmore (H) | Star Clusters in Mergers |
09:20 | 0:15 | Mengel (C) | Spectroscopy of Compact Star Clusters in NGC 4038/39 | |
09:40 | 0:15 | Gilbert (C) | Keck Infrared Spectroscopy of Star Clusters in Nearby Starbursts | |
YOUNG STAR CLUSTERS AND GLOBULAR CLUSTERS | 10:00 | 0:50 | DISCUSSION (led by Vacca) + COFFEE | |
TRIGGERING AND QUENCHING | 10:50 | 0:25 | Norman (R) | Triggering and Quenching: Physical Processes |
11:20 | 0:25 | Mihos (R) | Modeling Merger Induced Star Formation | |
11:50 | 0:15 | Lehnert (H) | Feedback by Supernovae and Superwinds | |
12:10 | 0:15 | van der Werf (C) | The Properties of Extreme Starbursts in Merging Galaxies | |
12:30 | 1:30 | LUNCH BREAK | ||
STAR FORMATION AND THE ISM | 14:00 | 0:25 | Sternberg (R) | The Interplay Between the ISM and Star Formation |
14:30 | 0:15 | Burkert (C) | Evidence for Disks in Elliptical Galaxies | |
14:50 | 0:25 | Scoville (C) | Starbursting in Spiral Arms and ULIRGs | |
15:20 | 0:15 | Solomon (C) | Starburst Mechanisms in Molecular Clouds: GMCs and ULIRGs | |
THE ISM-STARBURST CONNECTION | 15:35 | 1:00 | DISCUSSION (led by Harris) + COFFEE | |
MINI-DEBATE: Formation of Bulges and Ellipticals | 16:35 | 0:25 | Renzini (R) | Early: Through Bursts |
17:00 | 0:25 | Kauffmann (R) | Late: Through Mergers | |
17:25 | 1:00 | DISCUSSION (led by Aretxaga) | ||
18:30 | DINNER | |||
Wednesday, 13th | ||||
8:30 - 22:00 EXCURSION, HIKE, CONFERENCE DINNER | ||||
Thursday, 14th | ||||
SESSION | TIME | LENGTH | SPEAKER | TITLE |
GLOBAL PROPERTIES I | 09:00 | 0:25 | Charlot (R) | Modeling Stellar Populations at Low and High z |
09:30 | 0:25 | Schaerer (R) | Stellar Signatures in Integrated Spectra | |
10:00 | 0:15 | Gonzales Delgado (C) | Stellar Population of Nearby Starbursts | |
10:20 | 0:40 | COFFEE | ||
11:00 | 0:15 | Förster-Schreiber (H) | Star Formation Histories of Starbursts from ISO | |
11:20 | 0:15 | Fritze-von Alvensleben (H) | Chemical Evolution in Starbursts | |
11:40 | 0:15 | Dopita (C) | Chemical Abundances and Evolution in Nearby Starbursts | |
CAN WE DATE STARBURSTS? | 11:55 | 0:35 | DISCUSSION (led by Lançon) | |
12:30 | 1:30 | LUNCH BREAK | ||
GLOBAL PROPERTIES II | 14:00 | 0:15 | Poggianti (H) | Optical Spectra of Dusty Starbursts |
14:20 | 0:15 | Rigopoulou (H) | Star Formation Properties of ISOCAM Galaxies | |
14:40 | 0:15 | Moorwood (H) | Star forming Galaxies from z=2.2 H![]() |
|
15:00 | 0:15 | Graham (H) | The Metagalactic UV Background | |
15:20 | 0:40 | COFFEE | ||
16:00 | 0:15 | Moran (C) | Hard X-Rays from Starbursts Near and Far | |
16:20 | 0:15 | Thompson (C) | The Distribution of Star Formation Between Starbursts and Normal Galaxies from NICMOS Observations | |
16:40 | 0:50 | POSTER SUMMARIES | ||
HOW TO CORRECT FOR DUST EXTINCTION | 17:30 | 0:50 | DISCUSSION (led by Meurer) | |
18:30 | DINNER | |||
Friday, 15th | ||||
SESSION | TIME | LENGTH | SPEAKER | TITLE |
COSMIC STAR FORMATION HISTORY | 09:00 | 0:25 | Cesarsky (R) | ISOCAM survey results |
09:30 | 0:15 | Yan (H) | Emission Line Galaxies from NICMOS Surveys | |
09:50 | 0:15 | Hughes (H) | Results from SCUBA Surveys | |
10:10 | 0:15 | Bertoldi (H) | Results from MAMBO Surveys | |
10:30 | 0:40 | COFFEE | ||
11:10 | 0:15 | Carilli (H) | Deep Radio Surveys | |
11:30 | 0:15 | Sanders (C) | Nature of the ISOPHOT FIR Deep Field Sources | |
CONTRIBUTION OF DIFFERENT COMPONENTS TO FIR/SUBMM BACKGROUND | 11:45 | 0:40 | DISCUSSION: (led by Baker) | |
12:30 | 1:30 | LUNCH BREAK | ||
14:00 | 0:15 | Blain (C) | The History of Starburst Galaxies | |
DEBATE: How to best explore high-z star formation | 14:20 | 0:25 | Adelberger (R) | Cosmic SF history: The UV Takes it All |
14:45 | 0:25 | Franceschini (R) | Cosmic SF history: The Need for IR Observations | |
15:10 | 0:25 | Hasinger (R) | Cosmic SF history: The Need for X-ray Observations | |
15:35 | 1:30 | DISCUSSION (led by Genzel) + COFFEE | ||
SOC/LOC | Conference End | |||
18:00 | BUS DEPARTURE TO MUNICH |
Aretxaga | Young Stellar Populations in the Nuclear Regions of Nearby Radio Galaxies |
Baker | Dust Emission From The Lensed Lyman Break Galaxy cB58 |
Barden | CO Observations of Post-Starburst Galaxies |
Blum | The Stellar Content of Obscured Galactic Giant HII Regions |
Colina | Two-dimensional Integral-Field Spectroscopy of ULIRGs: Templates for High-Redshift SCUBA Sources |
Davies | Investigating ULIRGs in the Near-Infrared: Imaging & Spectroscopy |
Gilbert | Keck Infrared Spectroscopy of Star Clusters in Nearby Starbursts |
Harris | Submillimeter Line Emission from Active Galaxies |
Jogee | Circumnuclear Gas Transport and Star Formation Efficiency |
Lançon | Recognizing Post-Starburst Populations Near and Far |
Meurer | The Ultraviolet Properties of Ultraluminous Infrared Galaxies |
Spoon | 2-12 micron Spectrophotometry of Normal and Active Galaxies |
Tan | Super Star Clusters and Self Gravitating HII regions |
Tremonti | HST Ultraviolet Spectra of Local Starbursts: Benchmarks for High-Redshift Galaxies |
Veilleux | Merger Induced Super Starburst and Quasar Activity in the Local Universe |
or fax (49-89-3299-3569). Since, unfortunately, the MPE will be moving into a new building during the week before the conference, there is a small chance that our email service will be unavailable for short periods during this time. If you need to get in touch with us between 4-10 September, it is best to send the message to
as well as to the normal Ringberg account just to be sure we get it.
*************************************************************************** Itinerary Information ******************************************* Starburst Galaxies Near and Far Ringberg Castle, Germany 10 --- 15 September, 2000 ******************************************* Please send information by 01 September 2000 FLIGHT ARRIVAL INFORMATION: Arrival Date: Flight Number: Arrival Time: FLIGHT DEPARTURE INFROMATION: Departure Date: Flight Number: Departure Time: Will you be participating in the excursion/hike and conference dinner on Wednesday 13 September? ......... Number of persons ......... --------------------------------------------------------------------------
This marks the end of the Final Announcement. Click here to go back to the top of the page.
in order to get the book to Springer as quickly as possible. The page allocations are
Click here for LaTeX macros and example files.
All contributions should be submitted via e-mail to ringberg@mpe.mpg.de
To aid in the collation process, please provide the filename in the Subject line of the e-mail submission. The file naming convention is author.tex for the LaTeX files, and author_fig1.ps for contributed PostScript files. Examples:
Subject: lutz.tex Subject: tacconi_fig4.psThe reference file of any \psfig commands must accordingly match the author-coded postscript file name, e.g.:
\psfig{file=tacconi_fig4.ps,width=\textwidth}Please note that color figures will be reproduced in black and white!
This marks the end of the Proceedings Information and LaTeX Macros Section. Click here to go back to the top of the page.
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