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Stellar Evolution and White Dwarfs [Each Talk is 20 min + 10 min Discussion]
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Morning Session Chair: Sterl Phinney (Caltech)
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Session 1: Isolated White Dwarfs
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8:50am |
David Gross (KITP Director)
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Welcome |
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9:00am |
Falk Herwig (Keele Univ.)
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Stellar Evolution Update for <8 Solar Mass Stars and Maximum Mass that makes a White Dwarf |
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9:30am |
Kurtis Williams (Univ. Texas)
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White Dwarf Initial-Final Mass Relation from Open Clusters |
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10:00am |
James Liebert (Univ. of Arizona)
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New Results on White Dwarfs from Sloan |
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10:30am |
MORNING BREAK |
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Session 2: White Dwarfs in Binaries and Truncated Evolution
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11:00am |
Boris Gaensicke (Univ. of Warwick)
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Populations of (Pre) Cataclysmic Variables |
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11:30am |
Tom Marsh (Univ. of Warwick)
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Helium White Dwarfs in Binaries |
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12:00pm |
Ralf Napiwotzki (Univ. Hertfordshire)
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The Known Double White Dwarfs and Merger Rates |
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12:30pm |
LUNCH BREAK |
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Afternoon Session Chair: Rosanne DiStefano (Harvard, CfA)
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Session 3: White Dwarf Binaries in Contact
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2:00pm |
Gijs Nelemans (Radboud Univ.)
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Observational Implications for Common Envelope Evolution |
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2:30pm |
Sterl Phinney (Caltech)
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Dynamical Stability at the onset of Mass Transfer |
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3:00pm |
Ron Webbink (UIUC)
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Overview of Outcomes from White Dwarf Mergers |
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3:30pm |
AFTERNOON BREAK |
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Session 4: AM CVn Binaries: Helium Accretors
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4:00pm |
Christopher Deloye (NWU)
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Overview on He Accreting WDs: AM CVn's |
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4:30pm |
Lars Bildsten (KITP)
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Helium Shell Flashes and Faint Supernovae |
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5:00pm |
Bruno Leibundgut (ESO)
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Are the Subluminous Ia's Sub Chandra? |
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6:00pm |
SPECIAL EVENTS DINNER |
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8:00pm |
SHUTTLE TO BWSCI |
*Time may vary depending on end of dinner. |
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Accretion onto WDs, challenges.. [Each Talk is 20 min + 10 min Discussion]
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Morning Session Chair: Joe Patterson (Columbia Univ.)
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Session 1: Hydrogen Accretors: Unstable Burning
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9:00am |
Dean Townsley (Univ. of Chicago)
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Broad Views of Hydrogen Ignitions in CVs |
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9:30am |
Paula Szkody (Univ. Washington)
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Observed Properties of Accreting WDs in CVs |
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10:00am |
Sumner Starrfield (Arizona State Univ.)
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Excavation or Accretion from Classical Novae |
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10:30am |
MORNING BREAK |
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Session 2: Population Numbers from Weak Explosions
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11:00am |
Allen Shafter (San Diego)
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Accreting Populations Implied from Classical Novae in Nearby Galaxies |
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11:30am |
Marina Orio (Univ. Wisconsin)
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A View of M31 in the X-rays |
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12:00pm |
Jennifer Sokoloski (Columbia)
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Recurrent Novae, Symbiotics and RS Oph |
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12:30pm |
LUNCH BREAK |
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Afternoon Session Chair: Jennifer Sokoloski (Columbia Univ.)
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Session 3: Reaching Core Ignitions
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2:00pm |
Edward van den Heuvel (Univ. of Amsterdam)
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Binary Scenarios that may Achieve Core Ignitions |
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2:30pm |
Rosanne Di Stefano (Harvard, CfA)
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Are there enough Supersoft Sources to make the Ia's? |
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3:00pm |
Izumi Hachisu (Univ. Tokyo)
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Winds from Burning White Dwarfs |
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3:30pm |
AFTERNOON BREAK |
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Session 4: Ignition to Flames
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4:00pm |
Pierre Lesaffre (ENS/LRA)
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From Ignitions to Early Convective Phases: Convective Urca |
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4:30pm |
Jonathan Dursi (Univ. of Toronto)
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First Flames: Burning, Turbulence and Buoyancy |
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5:00pm |
Edward Brown (Michigan State Univ.)
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22Ne and Metallicity Effects |
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5:45pm |
SHUTTLE TO BWSCI |
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Day to Celebrate Ken Nomoto's 60th Birthday
[Each Talk is 30 min + 15 min Discussion]
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Morning Session Chair: Robert Kirshner (Harvard, CfA)
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9:00am |
Stan Woosley (UC Santa Cruz)
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Global Overview of Core Collapse + GRB |
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9:45am |
Friedel Thielemann (Univ. of Basel)
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From Accreting WDs to Explosion: The Story of W7 |
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10:30am |
MORNING BREAK |
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11:00am |
Wolfgang Hillebrandt (MPA, Garching)
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Current Models for Ia's |
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11:45am |
Alex Filippenko (UC Berkeley)
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Observational Confidence or Not ? |
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12:30pm |
LUNCH BREAK |
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Afternoon Session Chair: Craig Wheeler (Univ. Texas, Austin)
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2:00pm |
Jim Truran (Univ. of Chicago)
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Nucleosynthesis from Ias, Metal Poor Stars .. |
[Each Talk is 20 min + 10 min Discussion]
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2:45pm |
Paolo Mazzali (Trieste Obs)
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Supernovae and GRBs |
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3:15pm |
AFTERNOON BREAK |
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3:45pm |
Philipp Podsiadlowski (Univ. of Oxford)
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Electron-capture Supernovae and Accretion-induced Collapse
of ONeMg White Dwarfs |
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4:15pm |
Izumi Hachisu (Univ. Tokyo)
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Ken Nomoto's Contributions to Japanese Science |
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4:45pm |
Wolfgang Hillebrandt (MPA, Garching)
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Introducing Ken Nomoto |
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5:00pm |
Ken'ichi Nomoto (Univ. Tokyo)
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Closes Session |
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5:30pm |
SPECIAL EVENTS DINNER |
Dinner Speaker: Bob Kirshner |
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8:30pm |
SHUTTLE TO BWSCI |
*Time may vary depending on end of dinner. |
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Core Ignitions in Near Chandra Mass WDs [Each Talk is 20 min + 10 min Discussion]
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Session 1: Deflagrations to Detonations
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Morning Session Chair: Elaine Oran (Naval Research Lab)
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9:00am |
Fritz Roepke (MPA, Garching)
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Simulating Type Ia Supernovae: The Deflagration Model and Beyond |
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9:30am |
Tomasz Plewa (Univ. of Chicago)
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Thermonuclear Supernova: A Successful Failure |
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10:00am |
Vadim Gamezo (Naval Research Lab)
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Mechanisms for Deflagration-to-Detonation Transition in Type Ia Supernovae and Terrestrial Systems. |
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10:30am |
MORNING BREAK |
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Session 2: Deflagrations to Detonations (continued)
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11:00am |
Don Lamb (Univ. of Chicago)
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Gravitationally Confined Detonations |
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11:30am |
Daniel Kasen (John Hopkins)
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Overview of Theoretical Understanding of Type Ia Light Curves |
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12:00pm |
Ken'ichi Nomoto (Univ. Tokyo)
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Neutron-rich Nucleosynthesis in Type Ia's: Constraints from Near IR Nebular
Observations |
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12:30pm |
LUNCH BREAK |
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Afternoon Session Chair: Frank Timmes (LANL)
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Session 3: Spectral Insights
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2:00pm |
Paolo Mazzali (Trieste Obs)
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Constraints on Ia SN from Spectral Modeling |
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2:30pm |
Craig Wheeler (Univ. of Texas)
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Insights from Near IR Spectroscopy |
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3:00pm |
Carles Badenes (Rutgers)
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What has been learned about Type Ia SN from their Remnants |
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3:30pm |
AFTERNOON BREAK |
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Session 4: Spectral Insights..
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4:00pm |
Andy Howell (Univ. of Toronto)
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Is the Brightest Ia Sn really Super Chandra? |
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4:30pm |
David Branch (Univ. of Oklahoma)
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Comparative Direct Analysis of Type Ia Supernova Spectra |
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5:00pm |
Tom Matheson (NOAO/NGSC)
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Clues in Spectra for Luminosity Dependence |
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5:45pm |
WINE AND CHEESE RECEPTION |
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7:00pm |
SHUTTLE TO BWSCI |
*Time may vary depending on end of reception. |
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The Diversity and Changes? with Age [Each Talk is 20 min + 10 min Discussion]
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Session 1: New Insights
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Morning Session Chair: Dan Maoz (Tel Aviv Univ.)
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9:00am |
Doug Leonard (San Diego)
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What Polarimetry has taught us. |
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9:30am |
Mark Phillips (CTIO)
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The Peculiar SN 2005hk |
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10:00am |
Alicia Soderberg (Caltech)
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Observations of Ia SN that provide Evidence for Circumstellar Interactions |
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10:30am |
MORNING BREAK |
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Session 2: Type Ia rates and Properties: Galaxy Dependences
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11:00am |
Weldong Li (UC Berkeley)
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The Nearby SN Ia rate from the Lick Observatory Supernova Search |
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11:30am |
Saurabh Jha (Stanford)
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The Low-redshift Supernova Ia Sample |
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12:00pm |
Chris Pritchet (Univ. of Victoria)
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The Low Redshift Ia Rate as a Function of Galaxy Type |
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12:30pm |
LUNCH BREAK |
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Afternoon Session Chair: Avishay Gal-Yam (Caltech)
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Session 3: Cosmological Type Ia Results
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2:00pm |
Mark Sullivan (Univ. of Toronto)
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SNLS Results on Cosmology |
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2:30pm |
Michael Wood-Vasey (Harvard, CfA)
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ESSENCE Results: Similarity of SNeIa at Low and High Redshift |
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3:00pm |
Adam Riess (STScI)
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Lessons Learned from SNe Ia at z>1 |
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3:30pm |
AFTERNOON BREAK |
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Session 4: New Results
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4:00pm |
Peter Nugent (LBNL)
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The Environments of High and Low Luminosity SNe Ia |
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4:30pm |
Rollin Thomas (LBNL)
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New Results from the SNFactory |
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5:00pm |
Peter Garnavich (Notre Dame)
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New Results from SDSS |
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5:45pm |
SHUTTLE TO BWSCI |
Shuttle also available to SB Airport and SB Airbus, Goleta location. |
ABSTRACTS/POSTER PRESENTATION
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Shimon Asida (Hebrew Univ. of Jerusalem)
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Verification of an Advection-Diffusion-Reaction Flame Model for Type Ia Supernova Simulations |
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Carles Badenes (Rutgers)
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A Deep Chandra Observation of Kepler's Supernova Remnant: A Type Ia
Supernova with Circumstellar Interaction [abstract] |
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Stéphane Blondin (Harvard, CfA)
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Determining the Type, Redshift, and Phase of a Supernova Spectrum [abstract] |
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Nancy Elias (MPA, Garching)
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SN~2002cv: A Heavily Obscured Type Ia Event [abstract] |
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Robert Fisher (Univ. Chicago)
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Semi-Analytic Modelling of Nuclear Burning Bubbles and the
Implications for Physically Self-Consistent Initial Conditions
in Type Ia Supernova Simulations |
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Domingo García-Senz (UPC, Barcelona)
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Multidimensional Modelling of Type Ia Supernovae Explosions [abstract] |
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Nathan Hearn (Univ. Chicago)
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Simulating White Dwarf Merger Scenarios for Type Ia Supernovae |
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Falk Herwig (Keele Univ.)
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Multi-dimensional Simulations of Helium Shell Flash Convection [abstract] |
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Yutaka Ihara (Univ. Tokyo)
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Searching for a Companion Star of Tycho's Type Ia Supernova
with Optical Spectroscopic Observations [abstract] |
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George Jordan (Univ. Chicago)
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Three-Dimensional Simulations of the Deflagration Phase in the Gravitationally Confined Detonation Model of Type Ia Supernovae |
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Chiaki Kobayashi (NAOJ)
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Type Ia Supernova Progenitors, Elemental Abundance Ratios, and Cosmic Supernova Rate History |
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Casey Meakin (Univ. Chicago)
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Simulations of Detonations in the Context of the Gravitationally
Confined Detonation Model of Type Ia Supernovae |
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Tony Piro (UC Berkeley)
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Type Ia Progenitor Rotation: Accretion and Simmering [abstract] |
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Alexei Poludnenko (Univ. Chicago)
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From Seconds to Days: Modeling of Post-Explosion Evolution of Type Ia Supernova Explosions |
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Steven Rodney (Univ. Hawaii, IfA)
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Revisiting the SNIa Rate at z>1 [abstract] |
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Ivo Seitenzahl (Univ. Chicago)
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Detonation Criteria in the Gravitationally Confined Detonation Model of Type Ia Supernovae |
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Ken Shen (UCSB)
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Thermally Stable Nuclear Burning on Accreting White Dwarfs [abstract] |
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Stuart Sim (MPA, Garching)
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Light curves for lop-sided SNe Ia [abstract] |
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Vallery Stanishev (Stockholm Univ.)
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ESC Observations of the Peculiar Type Ia Supernova 2005hk [abstract] |
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Masaomi Tanaka (Univ. Tokyo)
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One and Three-Dimensional Modeling of Pre-maximum Spectra of Type Ia SNe [abstract] |
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Nozomu Tominaga (Univ. Tokyo)
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Nucleosynthesis in Jet-induced Supernovae [abstract] |
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Dean Townsley (Univ. Chicago)
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Flame Evolution During the Deflagration Phase of Type Ia Supernovae |
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Ju Zhang (Univ. Chicago)
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Low Mach Number Reactive Flow Solver For Modeling Core Convection in Type Ia Supernova Progenitors |
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Andrey Zhiglo (Univ. Chicago)
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Numerical Flame Propagation |
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