Abstract
We present the initial results from our GALEX program designed to obtain ultraviolet (UV) spectra of nearby core-collapse supernovae (SNe). Our first target, SN 2005ay in the nearby galaxy NGC 3938, is a typical member of the SN II-P subclass. Our spectra show remarkable similarity to those of the prototypical Type II-P SN 1999em, and resemble also Swift observations of the recent Type II-P SN 2005cs. Taken together, the observations of these three events trace the UV spectral evolution of SNe II-P during the first month after explosion, as required in order to interpret optical observations of high-redshift SNe II-P, and to derive cross-filter K-corrections. While still highly preliminary, the apparent UV homogeneity of SNe II-P bodes well for the use of these events as cosmological probes at high redshift.
Original language | English (US) |
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Pages (from-to) | L117-L120 |
Journal | Astrophysical Journal |
Volume | 685 |
Issue number | 2 PART 2 |
DOIs | |
State | Published - 2008 |
Keywords
- General
- Individual (SN 2005ay)
- Supernovae
- Ultraviolet
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science