... The majority of these stars belong to the spherical component of the Galaxy; they are present, sometimes in large numbers, in some globular clusters, where they are known as pulsating horizontal-branch stars. ...
... The majority of these stars belong to the spherical component of the Galaxy; they are present, sometimes in large numbers, in some globular clusters, where they are known as pulsating horizontal-branch stars. ...
... The majority of these stars belong to the spherical component of the Galaxy; they are present, sometimes in large numbers, in some globular clusters, where they are known as pulsating horizontal-branch stars. ...
... Astronomy of Russian Academy of Sciences gcvs@sai.msu.ru ftp ftp.sai.msu.su, /pub/groups/cluster/gcvs/gcvs/ (anonymous) http://www.sai.msu.su/groups/cluster/gcvs/gcvs/ Description: The fourth volume of the revised version 1.3 of the General Catalogue of ...
... V. , Clement C., Thompson M. The pulsation mode changes of the RR Lyrae type variable star V79 in the globular cluster M3 ... Kukarkin Centenary Conference: Variable Stars, the Galactic Halo and Galaxy formation", Abstract book, p.17-18, Moscow , 2009 ...
... cluster/gcvs/gcvs/vol1/ File Summary: ----------------------------------------------------------------- FileName Explanations ----------------------------------------------------------------- readme.txt This file vol1.pdf The text of the paper vol1.dat ...
... cluster/gcvs/gcvs/vol2/ File Summary: ----------------------------------------------------------------- FileName Explanations ----------------------------------------------------------------- readme.txt This file vol2.pdf The text of the paper vol2.dat ...
... long-period Cepheids, and young open star clusters (OSCs), as well as the H I and H ... known distances--classical Cepheids, open star clusters (OSC), and OB-associations ...
... Heiderman , A. L. ; Jogee , S. ; Bacon, D. J. ; :, Koposov , S. ; :, Zheng , X. Galaxy Evolution in Dense Environments: Properties of Interacting Galaxies in the Abell 901/902 Supercluster . ...