Works matching IS 17439213 AND DT 2011 AND VI 7 AND IP S281
Results: 80
Binary Paths to Type Ia Supernovae Explosions: the Highlights.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 341, doi. 10.1017/S1743921312015347
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On the Progenitor of SNR 0509-67.5.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 337, doi. 10.1017/S1743921312015335
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Light-Echo Spectrum Reveals the Type of Tycho Brahe's 1572 Supernova.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 335, doi. 10.1017/S1743921312015323
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Progenitor's Signatures in Type Ia Supernova Remnants.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 331, doi. 10.1017/S1743921312015311
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Type Ia Progenitor Hunt in Ancient Remnants.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 326, doi. 10.1017/S174392131201530X
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Survey for the Binary Progenitor in SN1006 and Update on SN1572.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 322, doi. 10.1017/S1743921312015293
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Late-Phase Observations of a Super-Chandrasekhar SN Ia.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 319, doi. 10.1017/S1743921312015281
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Optical Studies of the Low Velocity Gradient Type Ia Supernovae 2009an and 2009ig.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 316, doi. 10.1017/S174392131201527X
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Light Curve Models for SN 2009dc.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 314, doi. 10.1017/S1743921312015268
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Constraining the Properties of SNe Ia Progenitors from Light Curves.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 309, doi. 10.1017/S1743921312015256
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On the Progenitors of Type Ia Supernovae.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 303, doi. 10.1017/S1743921312015244
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Evidence for Circumstellar Material in Type Ia Supernovae via Sodium Absorption Features.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 299, doi. 10.1017/S1743921312015232
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Connecting Recurrent Novae to [Some] Type Ia Supernovae.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 291, doi. 10.1017/S1743921312015220
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Hydrostatic 12C Burning in CO WDs: the Simmering Phase of SNe Ia Progenitors.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 284, doi. 10.1017/S1743921312015219
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Properties of Carbon-Oxygen White Dwarf Merger Remnants.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 280, doi. 10.1017/S1743921312015207
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Constraining Type Ia Supernova Progenitors.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 275, doi. 10.1017/S1743921312015190
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Type Ia Supernovae from Sub-Chandrasekhar Mass White Dwarfs.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 267, doi. 10.1017/S1743921312015189
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Thermonuclear Supernova Explosions from White Dwarfs in Different Progenitor Systems.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 261, doi. 10.1017/S1743921312015177
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Type Ia Supernova Models and Progenitor Scenarios.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 253, doi. 10.1017/S1743921312015165
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Galactic Chemical Evolution in the Context of the Recently Revealed SNe Ia Delay Time Distribution.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 251, doi. 10.1017/S1743921312015153
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Single Degenerate Progenitors of Type Ia Supernovae.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 248, doi. 10.1017/S1743921312015141
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Type Ia Supernovae and Supersoft X-ray Sources.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 244, doi. 10.1017/S174392131201513X
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Population Synthesis of Type Ia SNe: Constraining Free Parameters from Observations.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 240, doi. 10.1017/S1743921312015128
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Type Ia Supernovae and the Uncertainties in their Progenitor Evolution.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 236, doi. 10.1017/S1743921312015116
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Two Distributions Shedding Light on Type Ia Supernovae Progenitors: Delay Times and G-Dwarf Metallicities.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 232, doi. 10.1017/S1743921312015104
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Theoretical Delay Time Distributions.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 225, doi. 10.1017/S1743921312015098
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Double White Dwarf Merger Rates.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 223, doi. 10.1017/S1743921312015086
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A Search for Type Ia Supernova Progenitors: the Central Stars of the Planetary Nebulae NGC 2392 and NGC 6026.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 221, doi. 10.1017/S1743921312015074
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Detecting Double Degenerate Progenitors of SNe Ia with LISA.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 217, doi. 10.1017/S1743921312015062
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Constraining White Dwarf Masses Via Apsidal Precession in Eccentric Double White Dwarf Binaries.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 213, doi. 10.1017/S1743921312015050
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He-accreting WDs as SNe Ia Progenitors.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 209, doi. 10.1017/S1743921312015049
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Helium Star Donor Channel to Type Ia Supernovae and Their Surviving Companion Stars.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 205, doi. 10.1017/S1743921312015037
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Modeling of the IR Light Curves of the Symbiotic Recurrent Nova T CrB.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 203, doi. 10.1017/S1743921312015025
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New Photometric Observations of RS Oph.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 201, doi. 10.1017/S1743921312015013
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Changes in the Dusty Environment of the Recurrent Nova RS Ophiuchi.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 199, doi. 10.1017/S1743921312015001
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The Asymmetric Outflow of RS Ophiuchi.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 195, doi. 10.1017/S1743921312014998
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The Mass of the White Dwarf in the Recurrent Nova CI Aquilae.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 193, doi. 10.1017/S1743921312014986
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The Helium Abundance in the Ejecta of U Scorpii.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 190, doi. 10.1017/S1743921312014974
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White Dwarf Masses and Accretion Rates of Recurrent Novae: an X-ray Perspective.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 186, doi. 10.1017/S1743921312014962
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X-ray Grating Observations of Recent Recurrent Novae.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 181, doi. 10.1017/S1743921312014950
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Novae and Accreting White Dwarfs as Progenitors of Type Ia Supernovae.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 172, doi. 10.1017/S1743921312014949
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Hydrodynamic Studies of the Evolution of Recurrent Novae to Supernova Ia Explosions.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 166, doi. 10.1017/S1743921312014937
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Symbiotic Stars as Possible Progenitors of SNe Ia: Binary Parameters and Overall Outlook.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 162, doi. 10.1017/S1743921312014925
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Recurrent Novae: What Do We Know about Them?
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 154, doi. 10.1017/S1743921312014913
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The Changing Nature of QU Carinae: SN Ia Progenitor or a Hoax?
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 149, doi. 10.1017/S1743921312014901
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Why are Supersoft X-ray Fluxes So Weak in Early-type Galaxies? – A Clue to Type Ia SNe Progenitors –.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 145, doi. 10.1017/S1743921312014895
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Obscuring Supersoft X-ray Sources in Stellar Winds.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 140, doi. 10.1017/S1743921312014883
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Ultra-soft Sources as Type Ia Supernovae Progenitors.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 136, doi. 10.1017/S1743921312014871
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The Appearance of Type Ia Supernova Progenitors: If Not SSSs, then What Do They Look Like?
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 132, doi. 10.1017/S174392131201486X
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Photometric Investigation of the Dwarf Nova OT J213806.6+261957 in Pegasus.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S281, p. 130, doi. 10.1017/S1743921312014858
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