Light Curves of Variable Stars in the Small Magellanic Cloud

Details Light Curves of Variable Stars in the Small Magellanic Cloud Light Curves of Variable Stars in the Small Magellanic Cloud

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aas...193.4610s&link_type=abstract

American Astronomical Society, 193rd AAS Meeting, #46.10; Bulletin of the American Astronomical Society, Vol. 30, p.1322

Astronomy and Astrophysics

Astronomy

Scientific paper

Light curves of variable stars in the northeast portion of the Small Magellanic Cloud have been constructed using B and V images obtained with a CCD camera on the Curtis Schmidt telescope at CTIO. The light curves confirm the existence of both first overtone and fundamental mode pulsators among the SMC Cepheids. We present representative light curves and discuss the locations of the variables in the color-magnitude diagram. Comparisons are made to Cepheids in the Galaxy.

Affiliated with

Also associated with

No associations

Rating

Light Curves of Variable Stars in the Small Magellanic Cloud 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 Light Curves of Variable Stars in the Small Magellanic Cloud, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Light Curves of Variable Stars in the Small Magellanic Cloud will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-994487