SN2009hd is a Highly-reddened Type IIP Supernova

Details SN2009hd is a Highly-reddened Type IIP Supernova SN2009hd is a Highly-reddened Type IIP Supernova

Jul 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.2118....1b&link_type=abstract

The Astronomer's Telegram, #2118

Astronomy and Astrophysics

Astronomy

1

Optical, Novae, Supernovae, Transients

Scientific paper

We used the Magellan Echellete spectrograph (MagE) on the Magellan/ Clay 6.5-m telescope to obtain a spectrum of SN2009hd in M66 (CBET #1867). The observations were taken on 2009 July 9.0 UT with a total exposure time of 900 sec. Inspection of the 1-d spectrum reveals a very red continuum dominated by broad H-alpha emission with a FWHM of about 6000 km/sec and a minimum that corresponds to a velocity of about 5800 km/sec.

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