Results 11 to 20 of about 349,394 (283)
THE INVESTIGATION OF THE CLASSICAL CEPHEID RT Aur PERIOD
The outcomes of the research into RT Aur period for the last 93 years are given in the article. New elements of changes in RT Aur brightness have been determined by the authors: J.D.max=2447890,265+3.7283116*E.
A. S. Kosinsky +5 more
doaj +1 more source
Sparse Logistic Regression for RR Lyrae versus Binaries Classification
RR Lyrae (RRL) stars are old, low-mass, radially pulsating variable stars in their core helium burning phase. They are popular stellar tracers and primary distance indicators since they obey well-defined period–luminosity relations in the near-infrared ...
Piero Trevisan +6 more
doaj +1 more source
Measurements of brightness of stars TX Crv, DP Cam, IRAS 17583+5150 opened in "IRAS" and "HIPPARCOS" experiments are carried out using negatives of the Odessa observatory.
A. P. Solonovich +2 more
doaj +1 more source
SOME RESULTS OF THE U CrB OBSERVATIONS IN 1856 - 2007
Historical results over of photometry of eclipsing variable star U CrB (type of EA / SD) are brought after 1856 - 2007. Authors suppose that in the system U CrB there is a trade-out by a substance between components.
V. D. Grigorenko +3 more
doaj +1 more source
Extrasolar planets and possibility of the life appearance
Review opened to November, 2006 extrasolar planetary ...
I. Kuzenkov +3 more
doaj +1 more source
Finding the most variable stars in the Orion Belt with the All Sky Automated Survey [PDF]
We look for high-amplitude variable young stars in the open clusters and associations of the Orion Belt. We use public data from the ASAS-3 Photometric V-band Catalogue of the All Sky Automated Survey, infrared photometry from the 2MASS and IRAS ...
Acke +137 more
core +3 more sources
Investigating Stellar Variability in the Open Cluster Region NGC 381
We study variable stars in the field of the open cluster NGC 381 using photometric data observed over 27 nights and identify a total of 57 variable stars, six of which are member stars. The variable stars are classified based on their periods, amplitudes,
Jayanand Maurya +3 more
doaj +1 more source
SiO Masers In Variable-Stars [PDF]
NSF MPS 05070 ...
Blair, Guy N., Dickinson, Dale F.
core +1 more source
Proper identification of RR Lyrae Stars brighter than 12.5 mag [PDF]
RR Lyrae stars are of great importance for investigations of Galactic structure. However, a complete compendium of all RR-Lyraes in the solar neighbourhood with accurate classifications and coordinates does not exist to this day.
Altmann +13 more
core +1 more source

