A SECOND CASE OF VARIABLE Na I D LINES IN A HIGHLY REDDENED TYPE Ia SUPERNOVA

作者：Blondin S^*; Prieto J L; Patat F; Challis P; Hicken M; Kirshner R P; Matheson T; Modjaz M

来源：Astrophysical Journal, 2009, 693(1): 207-215.

DOI：10.1088/0004-637X/693/1/207

• circumstellar matter
• dust
• extinction
• supernovae: general

Recent high-resolution spectra of the Type Ia supernova SN 2006X have revealed the presence of time-variable and blueshifted Na I D features, interpreted by Patat et al. as originating in circumstellar material within the progenitor system. The variation seen in SN 2006X induces relatively large changes in the total Na I D equivalent width (Delta EW similar to 0.5 angstrom in just over two weeks) that would be detectable at lower resolutions. We have used a large data set comprising 2400 low-resolution spectra of 450 Type Ia supernovae (SNe Ia) obtained by the CfA Supernova Program to search for variable Na I D features. Out of the 31 SNe Ia (including SN 2006X) in which we could have detected similar EW variations, only one other (SN 1999cl) shows variable Na I D features, with an even larger change over a similar similar to 10 day timescale (Delta EW = 1.66 /- 0.21 angstrom). Interestingly, both SN 1999cl and SN 2006X are the two most highly reddened objects in our sample, raising the possibility that the variability is connected to dusty environments.

• 出版日期2009-3-1