Ultra-short period Cepheids in the LMC

Details Ultra-short period Cepheids in the LMC Ultra-short period Cepheids in the LMC

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ssrv...27..443c&link_type=abstract

(International Astronomical Union, Colloquium on Stellar Hydrodynamics, 58th, Los Alamos, N. Mex., Aug. 12-15, 1980.) Space Scie

Astronomy and Astrophysics

Astronomy

1

Cepheid Variables, Magellanic Clouds, Periodic Variations, Astronomical Catalogs, Light Curve, Star Distribution

Scientific paper

Six Cepheids in the Large Magellanic Cloud have been discovered with periods less than one day. They lie at the faint, blue end of the instability strip as would be expected but form a separate Period-Luminosity relation from that for normal Cepheids. Membership in the LMC is based upon the existence of the P-L relationship. Several of the variables have uncertain periods although all apparently have periods under one day. One additional variable has tentatively been identified as a bright Anomalous Cepheid.

Affiliated with

Also associated with

No associations

Rating

Ultra-short period Cepheids in the LMC 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 Ultra-short period Cepheids in the LMC, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ultra-short period Cepheids in the LMC will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-758270