Nearby Supernova Factory Observations of SN 2005gj: Another Type Ia Supernova in a Massive Circumstellar Envelope

By G. Aldering, P. Antilogus, S. Bailey, C. Baltay, A. Bauer, N. Blanc, S. Bongard, Y. Copin, E. Gangler, S. Gilles and 16 more. 2006

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We report Nearby Supernova Factory observations of SN 2005gj, the second confirmed case of a ``hybrid'' Type Ia/IIn supernova, which we interpret as the explosion of a white dwarf interacting with a circumstellar medium. Our early-phase photometry of SN 2005gj shows that the interaction is much stronger than for the prototype, SN 2002ic. Our first spectrum shows a hot continuum with broad and narrow Hα emission. Later spectra, spanning over 4 months from outburst, show clear Type Ia features combined with broad and narrow Hγ, Hβ, Hα, and He I λλ5876, 7065 in emission. At higher resolution, P Cygni profiles are apparent. Surprisingly, we also observe an inverted P Cygni profile for [O III] λ5007. We find that the light curve and measured velocity of the unshocked circumstellar material imply mass loss as recently as 8 years ago. The early light curve is well described by a flat radial density profile for the circumstellar material. However, our decomposition of the spectra into Type Ia and shock emission components allows for little obscuration of the supernova, suggesting an aspherical or clumpy distribution for the circumstellar material. We suggest that the emission-line velocity profiles arise from electron scattering rather than the kinematics of the shock. This is supported by the inferred high densities and the lack of evidence for evolution in the line widths. Ground- and space-based photometry and Keck spectroscopy of the host galaxy are used to ascertain that the host galaxy has low metallicity (Z/Z☉ < 0.3; 95% confidence) and that this galaxy is undergoing a significant star formation event that began roughly 200 ± 70 Myr ago. We discuss the implications of these observations for progenitor models and cosmology using Type Ia supernovae.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

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STELLAR AND PLANETARY PROPERTIES OF K2 CAMPAIGN 1 CANDIDATES AND VALIDATION OF 17 PLANETS, INCLUDING A PLANET RECEIVING EARTH-LIKE INSOLATION (2015, neutral): “Details of the SNIFS reduction, including dark, bias, and flat-field corrections, cleaning the data of bad pixels and cosmic rays, and extraction of the one-dimensional spectrum are described in Bacon et al. (2001) and Aldering et al. (2006).”
TYPE Ia SUPERNOVAE STRONGLY INTERACTING WITH THEIR CIRCUMSTELLAR MEDIUM (2013, background): “The two best-studied objects in this class are SNe 2002ic and 2005gj (Hamuy et al. 2003; Deng et al. 2004; Kotak et al. 2004; Wang et al. 2004; Wood-Vasey et al. 2004; Aldering et al. 2006; Prieto et al. 2007).”
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On the Progenitor of SN 2005gl and the Nature of Type IIn Supernovae (2006, background): “…SNe Ia/IIn, including the prototype SN 2002ic (Hamuy et al. 2003; WoodVasey et al. 2004) along with its recent (SN 2005gj [Prieto et al. 2005; Aldering et al. 2006]) and past (SN 1997cy [Germany et al. 2000; Turrato et al. 2000] and SN 1999E [Filippenko 2000; Rigon et al. 2003]) clones…”
Observational Clues to the Progenitors of Type Ia Supernovae (2013, background): “Until recently, H and He in emission was reported in only two SNe Ia: SN 2002ic (Hamuy et al. 2003) and SN 2005gj (Aldering et al. 2006, Prieto et al. 2007).”
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