Spectroscopic Identification of Nova M31 2008-05c

Details Spectroscopic Identification of Nova M31 2008-05c Spectroscopic Identification of Nova M31 2008-05c

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1568....1r&link_type=abstract

The Astronomer's Telegram, #1568

Astronomy and Astrophysics

Astronomy

2

Optical

Scientific paper

On 2008 June 8.60 UT a spectrum of Nova M31 2008-05c (ATel#1546) was obtained with the Low-Resolution Imager and Spectrograph (LRIS) on the Keck-I 10-m telescope. Observations were performed through heavy cloud cover using the 400/3400 grism (6.5 angstrom FWHM) and 400/8500 grating (5.6 angstrom FWHM) and exposures of 2x920s and 2x900s, respectively. The spectrum shows strong Balmer lines with velocity widths of 1800+-100 km/s.

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