The Peculiar SN 2005hk: Do Some Type Ia Supernovae Explode as Deflagrations?* ** ***

ABSTRACT We present extensive \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $u^{\prime }g^{\prime }r^{\prime }i^{\prime }BVRIYJHK_{s}$ \end{document} photometry and optical spectroscopy of the Type Ia supernova (SN) 2005hk. These data reveal that SN 2005hk was nearly identical in its observed properties to SN 2002cx, which has been called “the most peculiar known Type Ia supernova.” Both supernovae exhibited high‐ionization SN 1991T–like premaximum spectra, yet low peak luminosities like that of SN 1991bg. The spectra reveal th...

[1]  Alexei V. Filippenko,et al.  Optical spectra of supernovae , 1997 .

[2]  Harry L. Shipman,et al.  White Dwarfs: Cosmological and Galactic Probes , 2005 .

[3]  M. Reinecke,et al.  Three-dimensional modeling of type Ia supernovae - The power of late time spectra , 2005, astro-ph/0504317.

[4]  P. Berlind,et al.  Chemistry and Star Formation in the Host Galaxies of Type Ia Supernovae , 2005 .

[5]  J. P. Huchra,et al.  Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant , 1998, astro-ph/9801080.

[6]  The progenitors of subluminous type Ia supernovae , 2001, astro-ph/0105246.

[7]  Constraints on the progenitor systems of type Ia supernovae , 2005, astro-ph/0506415.

[8]  S. E. Persson,et al.  Optical and Infrared Photometry of the Type Ia Supernovae 1991T, 1991bg, 1999ek, 2001bt, 2001cn, 2001cz, and 2002bo , 2004, astro-ph/0409036.

[9]  William A. Fowler,et al.  Nucleosynthesis in Supernovae. , 1960 .

[10]  Caltech,et al.  SN 2002cx: The Most Peculiar Known Type Ia Supernova , 2003, astro-ph/0301428.

[11]  A. S. Fruchter,et al.  Timescale Stretch Parameterization of Type Ia Supernova B-Band Light Curves , 2001, astro-ph/0104382.

[12]  D. Kasen Secondary Maximum in the Near-Infrared Light Curves of Type Ia Supernovae , 2006, astro-ph/0606449.

[13]  Steve Gunnels,et al.  The Las Campanas Infrared Survey Camera , 2002 .

[14]  Theoretical light curves for deflagration models of Type Ia supernova , 2006, astro-ph/0603036.

[15]  P. Nugent Evidence for a Spectroscopic Sequence Among SNe IA , 1995 .

[16]  P. Astier,et al.  SALT : a spectral adaptive light curve template for type Ia supernovae , 2005 .

[17]  D. Schlegel,et al.  Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds , 1998 .

[18]  R. Kirshner,et al.  SN 1991T: Further Evidence of the Heterogeneous Nature of Type IA Supernovae , 1992 .

[19]  M. Fukugita,et al.  The Sloan Digital Sky Survey Photometric System , 1996 .

[20]  Bohdan Paczynski,et al.  Small-telescope astronomy on global scales : IAU Colloquium 183, Proceedings of a Colloquium held in Kenting, Taiwan 4-8 January 2001 , 2001 .

[21]  R. Ellis,et al.  Measurements of $\Omega$ and $\Lambda$ from 42 high redshift supernovae , 1998, astro-ph/9812133.

[22]  Wendy L. Freedman,et al.  The Carnegie Supernova Project: The Low‐Redshift Survey , 2005, astro-ph/0512039.

[23]  Kevin Krisciunas,et al.  Hubble Diagrams of Type Ia Supernovae in the Near-Infrared , 2003, astro-ph/0312626.

[24]  Robert Lupton,et al.  A Modified Magnitude System that Produces Well-Behaved Magnitudes, Colors, and Errors Even for Low Signal-to-Noise Ratio Measurements , 1999, astro-ph/9903081.

[25]  S. Woosley SN 1987A: After the Peak , 1988 .

[26]  Elaine S Oran,et al.  Deflagrations and detonations in thermonuclear supernovae. , 2004, Physical review letters.

[27]  et al,et al.  The Sloan Digital Sky Survey Photometric Camera , 1998, astro-ph/9809085.

[28]  M. Phillips,et al.  Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant , 1998, astro-ph/9805201.

[29]  A. Filippenko,et al.  CCD photometry of three Type Ia supernovae: V, R, and I light curves , 1993 .

[30]  R. Thomas,et al.  Spectral Consequences of Deviation from Spherical Composition Symmetry in Type Ia Supernovae , 2001, astro-ph/0107464.

[31]  Arlo U. Landolt,et al.  UBVRI Photometric Standard Stars in the Magnitude Range 11 , 1992 .

[32]  W. Arnett Type I supernovae. I. Analytic solutions for the early part of the light curve , 1982 .

[33]  C. Stubbs,et al.  Optical Photometry of the Type I[CLC]a[/CLC] Supernova 1999[CLC]ee[/CLC] and the Type I[CLC]b[/CLC]/[CLC]c[/CLC] Supernova 1999[CLC]ex[/CLC] in IC 5179 , 2002 .

[34]  Spectropolarimetry of the Peculiar Type Ia Supernova 2005hk , 2006, astro-ph/0603083.

[35]  Jan Peters,et al.  SN 1991bg - A type Ia supernova with a difference , 1993 .

[36]  R. Bacon,et al.  Overview of the Nearby Supernova Factory , 2002, SPIE Astronomical Telescopes + Instrumentation.

[37]  Nicholas B. Suntzeff,et al.  The Hubble diagram of the Calan/Tololo type IA supernovae and the value of HO , 1996 .

[38]  A. G. Alexei,et al.  OBSERVATIONAL EVIDENCE FROM SUPERNOVAE FOR AN ACCELERATING UNIVERSE AND A COSMOLOGICAL CONSTANT , 1998 .

[39]  L. Ho,et al.  The subluminous spectroscopically peculiar type Ia supernova 1991bg in the elliptical galaxy NGC 4374 , 1992 .

[40]  Lifan Wang,et al.  Could There Be a Hole in Type Ia Supernovae? , 2003, astro-ph/0311009.

[41]  Nucleosynthesis in multi-dimensional SN Ia explosions , 2004, astro-ph/0406281.

[42]  An early-time infrared and optical study of the Type Ia Supernova 1998bu in M96 , 2000, astro-ph/0007022.

[43]  J. Wheeler,et al.  Hubble's constant and exploding carbon–oxygen white dwarf models for Type I supernovae , 1985, Nature.

[44]  Wesley Ketchum,et al.  Comparative Direct Analysis of Type Ia Supernova Spectra , 2006 .

[45]  S. Jha,et al.  The Luminosity of SN 1999by in NGC 2841 and the Nature of “Peculiar” Type Ia Supernovae , 2001, astro-ph/0105490.

[46]  Alan Uomoto,et al.  The [CLC][ITAL]u[/ITAL][/CLC][arcmin]′[CLC][ITAL]g[/ITAL][/CLC][arcmin]′[CLC][ITAL]r[/ITAL][/CLC][arcmin]′[CLC][ITAL]i[/ITAL][/CLC][arcmin]′[CLC][ITAL]z[/ITAL][/CLC][arcmin]′ Standard-Star System , 2002 .

[47]  RETROCAM: A VERSATILE OPTICAL IMAGER FOR SYNOPTIC STUDIES , 2005, astro-ph/0502274.

[48]  A New Method to Calibrate the Magnitudes of Type Ia Supernovae at Maximum Light , 2006, astro-ph/0603407.

[49]  S. Jha,et al.  Late-Time Spectroscopy of SN 2002cx: The Prototype of a New Subclass of Type Ia Supernovae , 2006, astro-ph/0602250.

[50]  Danielle Alloin,et al.  Stellar candles for the extragalactic distance scale , 2003 .

[51]  M. Phillips,et al.  Evidence for a Spectroscopic Sequence among Type Ia Supernovae , 1995, astro-ph/9510004.

[52]  R. Thomas,et al.  Reading the Spectra of the Most Peculiar Type Ia Supernova 2002cx , 2004, astro-ph/0408130.

[53]  M. Phillips,et al.  The reddening-free decline rate versus luminosity relationship for type ia supernovae , 1999, astro-ph/9907052.

[54]  Type Ia supernova diversity in three-dimensional models , 2005, astro-ph/0506107.

[55]  W. M. Wood-Vasey,et al.  Using Line Profiles to Test the Fraternity of Type Ia Supernovae at High and Low Redshifts , 2005, astro-ph/0510089.

[56]  Walter A. Siegmund,et al.  The 2.5 m Telescope of the Sloan Digital Sky Survey , 2006, astro-ph/0602326.

[57]  B. F. Madore,et al.  The Discovery of Cepheids and a New Distance to NGC 2841 Using the Hubble Space Telescope , 2001 .

[58]  Optical Light Curve of the Type Ia Supernova 1998bu in M96 and the Supernova Calibration of the Hubble Constant , 1998, astro-ph/9811205.

[59]  R. Ellis,et al.  The Rise Time of Type Ia Supernovae from the Supernova Legacy Survey , 2006, astro-ph/0607363.

[60]  William Press,et al.  A Precise Distance Indicator: Type Ia Supernova Multicolor Light-Curve Shapes , 1996, astro-ph/9604143.

[61]  Nicholas B. Suntzeff,et al.  A Hubble diagram of distant type IA supernovae , 1993 .

[62]  M. Thomas,et al.  Optical and Infrared Photometry of the Unusual Type Ia Supernova 2000cx , 2002, astro-ph/0212543.

[63]  E. Baron,et al.  Detectability of Mixed Unburnt C+O in Type Ia Supernova Spectra , 2003, astro-ph/0303627.

[64]  R. Stothers Cosmic Explosions , 1965, Nature.

[65]  Consistent estimates of ⁵⁶Ni yields for type Ia supernovae , 2006, astro-ph/0609232.

[66]  A. Riess,et al.  The Rise Time of Nearby Type Ia Supernovae , 1999, astro-ph/9907037.

[67]  J. Mathis,et al.  The relationship between infrared, optical, and ultraviolet extinction , 1989 .

[68]  W. Arnett On the theory of type I supernovae. , 1979 .

[69]  D. Schlegel,et al.  The peculiar type Ia SN 1991T : detonation of a white dwarf ? , 1992 .

[70]  Monte Carlo Simulations of Type Ia Supernova Observations in Supernova Surveys , 2000, astro-ph/0006291.

[71]  S. E. Persson,et al.  A New System of Faint Near-Infrared Standard Stars , 1998 .

[72]  Lower limits on the Hubble constant from models of type Ia supernovae , 2004, astro-ph/0410686.