How much H and He is ‘hidden’ in SNe Ib/c? – I. Low-mass objects
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P. Mazzali | W. Hillebrandt | S. Taubenberger | K. Nomoto | D. Sauer | S. Hachinger | P. Mazzali | Ken'ichi Nomoto | Daniel Sauer
[1] P. Deuflhard. Newton Methods for Nonlinear Problems: Affine Invariance and Adaptive Algorithms , 2011 .
[2] David Polishook,et al. SN 2011dh: DISCOVERY OF A TYPE IIb SUPERNOVA FROM A COMPACT PROGENITOR IN THE NEARBY GALAXY M51 , 2011, 1106.3551.
[3] Physics,et al. SN 2009jf: a slow-evolving stripped-envelope core-collapse supernova , 2011, 1106.3030.
[4] N. Langer,et al. Runaway stars as progenitors of supernovae and gamma-ray bursts , 2011, 1103.1877.
[5] S. Valenti,et al. The He-rich stripped-envelope core-collapse supernova 2008ax , 2011, 1101.1824.
[6] Hydrogen and helium in the late phase of SNe IIb , 2010, 1007.1881.
[7] E. Baron,et al. SEARCHING FOR HYDROGEN IN TYPE Ib SUPERNOVAE , 2010, 1006.1359.
[8] S. Woosley,et al. TYPE Ib/c SUPERNOVAE IN BINARY SYSTEMS. I. EVOLUTION AND PROPERTIES OF THE PROGENITOR STARS , 2010, 1004.0843.
[9] R. Foley,et al. THE TRANSITIONAL STRIPPED-ENVELOPE SN 2008ax: SPECTRAL EVOLUTION AND EVIDENCE FOR LARGE ASPHERICITY , 2010, 1001.2775.
[10] P. Brown,et al. MULTI-WAVELENGTH PROPERTIES OF THE TYPE IIb SN 2008ax , 2009, 0909.0967.
[11] Stephen J. Smartt,et al. Progenitors of Core-Collapse Supernovae , 2009, 0908.0700.
[12] Rolf Walder,et al. The different progenitors of type Ib, Ic SNe, and of GRB , 2009, 0906.2284.
[13] Peter R. Young,et al. CHIANTI - an atomic database for emission lines. IX. Ionization rates, recombination rates, ionization equilibria for the elements hydrogen through zinc and updated atomic data , 2009 .
[14] L. A. Antonelli,et al. The Metamorphosis of Supernova SN 2008D/XRF 080109: A Link Between Supernovae and GRBs/Hypernovae , 2008, Science.
[15] Yuri Ralchenko,et al. Electron-impact excitation and ionization cross sections for ground state and excited helium atoms , 2008 .
[16] E. Ofek,et al. The Type IIb SN 2008ax: spectral and light curve evolution , 2008, 0805.1914.
[17] D. Morton,et al. A Multiplet Table for Neutral Helium (4He I) with Transition Rates , 2007 .
[18] G. Martínez-Pinedo,et al. Theory of core-collapse supernovae , 2006, astro-ph/0612072.
[19] Tokyo,et al. The properties of the 'standard' type Ic supernova 1994I from spectral models , 2006, astro-ph/0604293.
[20] D. Branch,et al. Hydrogen in Type Ic Supernovae? , 2006, astro-ph/0604047.
[21] D. Fox,et al. A non-spherical core in the explosion of supernova SN 2004dj , 2006, Nature.
[22] M. Turatto,et al. 1604-2004: Supernovae as Cosmological Lighthouses , 2005 .
[23] Anthony Mezzacappa,et al. ASCERTAINING THE CORE COLLAPSE SUPERNOVA MECHANISM: The State of the Art and the Road Ahead , 2005 .
[24] T. Piran. The physics of gamma-ray bursts , 2004, astro-ph/0405503.
[25] Garching,et al. Abundance stratification in Type Ia supernovae - I. The case of SN 2002bo , 2004, astro-ph/0409342.
[26] J. Cuby,et al. Optical and Infrared Spectroscopy of SN 1999ee and SN 1999ex , 2002, astro-ph/0203491.
[27] N. M. Cann,et al. Quadrupole oscillator strengths for the helium isoelectronic sequence: n 1S-m 1D, n 3S-m 3D, n 1P-m 1P, and n 3P-m 3P transitions with n <7 and m <7 , 2002 .
[28] L. Lucy. Monte Carlo transition probabilities , 2001 .
[29] G. Lach,et al. Forbidden transitions in the helium atom , 2001, physics/0105110.
[30] P. Mazzali,et al. Can Differences in the Nickel Abundance in Chandrasekhar-Mass Models Explain the Relation between the Brightness and Decline Rate of Normal Type Ia Supernovae? , 2000, astro-ph/0009490.
[31] J. Cassinelli,et al. Introduction to Stellar Winds by Henny J. G. L. M. Lamers , 1999 .
[32] J. Cassinelli,et al. Introduction to Stellar Winds , 1999 .
[33] A. MacFadyen,et al. Collapsars: Gamma-Ray Bursts and Explosions in “Failed Supernovae” , 1998, astro-ph/9810274.
[34] C. McKee,et al. The Expulsion of Stellar Envelopes in Core-Collapse Supernovae , 1998, astro-ph/9807046.
[35] D. G. Hummer,et al. Recombination of helium-like ions – I. Photoionization cross-sections and total recombination and cooling coefficients for atomic helium , 1998 .
[36] D. Schlegel,et al. Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds , 1998 .
[37] L. Lucy,et al. The 1.05‐μm feature in the spectrum of the Type Ia supernova 1994D: He in SNe Ia? , 1998 .
[38] D. Schlegel,et al. Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds , 1997, astro-ph/9710327.
[39] H. Mason,et al. CHIANTI - an atomic database for emission lines - I. Wavelengths greater than 50 Å , 1997 .
[40] Alejandro Clocchiatti,et al. SN 1994I: Disentangling He i Lines in Type IC Supernovae , 1996 .
[41] Chien Y. Peng,et al. UBVRI Photometry of the Type IC SN 1994I in M51 , 1996 .
[42] Thomas Matheson,et al. The Type Ic Supernova 1994I in M51: Detection of Helium and Spectral Evolution , 1995 .
[43] Shiomi Kumagai,et al. Theoretical light curves for the type IC supernova SN 1994I , 1994 .
[44] K. Nomoto,et al. A carbonoxygen star as progenitor of the type Ic supernova 1994I , 1994, Nature.
[45] D. Swartz. Charge transfer in helium-rich supernova plasma , 1994 .
[46] K. Nomoto,et al. Theoretical light curves of the type IIB supernova 1993J , 1993 .
[47] S. Woosley. Gamma-ray bursts from stellar mass accretion disks around black holes , 1993 .
[48] R. Janev,et al. Atomic and plasma-material interaction processes in controlled thermonuclear fusion , 1993 .
[49] C. Fransson,et al. Gamma-Ray Deposition and Nonthermal Excitation in Supernovae , 1992 .
[50] Ulrich Nowak,et al. A Family of Newton Codes for Systems of Highly Nonlinear Equations. , 1992 .
[51] L. Lucy. Nonthermal excitation of helium in type Ib supernovae , 1991 .
[52] R. McCray,et al. Energy degradation of fast electrons in hydrogen gas , 1991 .
[53] K. Nomoto,et al. Low-mass helium star models for Type Ib supernovae : light curves, mixing, and nucleosynthesis , 1990 .
[54] J. Graham. Radioactive ionization of the envelope of SN 1987A , 1988 .
[55] M. Seaton,et al. Atomic data for opacity calculations. VII. Energy levels, f values and photoionisation cross sections for He-like ions , 1987 .
[56] R. Kirshner,et al. The early spectral phase of type Ib supernovae - Evidence for helium , 1987 .
[57] G. Rybicki,et al. The Sobolev approximation for line formation with continuous opacity , 1985 .
[58] L. Lucy,et al. Multiline Transfer and the Dynamics of Stellar Winds , 1985 .
[59] B. Pagel,et al. Stellar atmospheres , 1978, Nature.
[60] S. Bashkin,et al. Atomic energy levels and Grotrian diagrams , 1975 .
[61] W. Arnett. Advanced evolution of massive stars. V. Neon burning , 1974 .
[62] R. Gould. Energy loss of fast electrons and positrons in a plasma , 1972 .
[63] W.K. (Bill) Peterson,et al. Tables of secondary-electron-production cross sections , 1972 .
[64] H. Habing,et al. Heating of the Interstellar Medium by X-Rays and by Cosmic Rays , 1971 .
[65] D. Mihalas,et al. Statistical Equilibrium Model Atmospheres for Early-Type Stars. III. Hydrogen and Helium Continua , 1968 .
[66] W. Lotz. Electron Impact Ionization Cross Sections and Ionization Rate Coefficients for Atoms and Ions , 1967 .