Photométrie Photoélectrique d'Etoiles Variables Brillantes

Details Photométrie Photoélectrique d'Etoiles Variables Brillantes Photométrie Photoélectrique d'Etoiles Variables Brillantes

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986bicds..30...79s&link_type=abstract

Bulletin d'Information du Centre de Donnees Stellaires, Vol. 30, p.79

Physics

Scientific paper

A statistical study of variable stars brighter than m = 10 at maximum has been undertaken. It is based upon the Fourth Edition of the General Catalogue of Variable Stars (Moscow, 1985), first part, which contains the variables located in the constellations Andromeda, Antlia, etc. to Orion. For a total of 18151 stars, 2207 (12%) are brighter than m = 10 at maximum. 1240 out of this number (i.e. more than half) have been observed photoelectrically.

Affiliated with

Also associated with

No associations

Rating

Photométrie Photoélectrique d'Etoiles Variables Brillantes 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 Photométrie Photoélectrique d'Etoiles Variables Brillantes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Photométrie Photoélectrique d'Etoiles Variables Brillantes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1281493