A Dramatic Change in the H-alpha Emission and Continuum Flux of S Doradus

Details A Dramatic Change in the H-alpha Emission and Continuum Flux of S Doradus A Dramatic Change in the H-alpha Emission and Continuum Flux of S Doradus

Apr 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2560....1r&link_type=abstract

The Astronomer's Telegram, #2560

Astronomy and Astrophysics

Astronomy

Optical, Request For Observations, Variables, Stars

Scientific paper

S Dor is a prototypical Luminous Blue Variable and is one of the brightest objects in the Large Magellanic Cloud. The star's photometric history over the last century is described by van Genderen et al. (1997) in terms of a very-long-term and a quasi-periodic (7 year) variation. The faintest V-magnitude (V=11.3) was observed in 1965, while the brightest V-magnitude (V=8.8) was observed in 2006 by the All Sky Automated Survey (Pojmanski 2002).

Affiliated with

Also associated with

No associations

Rating

A Dramatic Change in the H-alpha Emission and Continuum Flux of S Doradus 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 A Dramatic Change in the H-alpha Emission and Continuum Flux of S Doradus, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Dramatic Change in the H-alpha Emission and Continuum Flux of S Doradus will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1311148