Spectroscopic identification of the high-amplitude variable star in Leo

Details Spectroscopic identification of the high-amplitude variable star in Leo Spectroscopic identification of the high-amplitude variable star in Leo

Nov 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atel..951....1r&link_type=abstract

The Astronomer's Telegram, #951

Astronomy and Astrophysics

Astronomy

1

Optical, Transients, Variables

Scientific paper

We report on follow-up spectroscopy of the high-amplitude variable star in Leo (see Christensen et al., CBET#746) with the COSMIC spectrograph mounted on the Hale-5m telescope at Palomar Observatory. Observations were performed on UT 2006 November 21.55 and covered a wavelength range from 4000 to 8200 Angstrom with a resolution of ~8 Angstrom. The spectrum shows a very blue continuum and prominent Balmer absorption lines (H_epsilon to H_alpha) together with a weak HeI P-Cygni profile around 5876 Angstrom.

Affiliated with

Also associated with

No associations

Rating

Spectroscopic identification of the high-amplitude variable star in Leo does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Spectroscopic identification of the high-amplitude variable star in Leo, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectroscopic identification of the high-amplitude variable star in Leo will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1311631