Results 11 to 20 of about 51,534 (310)
Measurements of brightness of stars 1AL Ari, FM Leo, LL Aqr, V1125 Tau, V1366 Ori opened in ”HIPPARCOS” experiment are carried out using negatives of the Odessa observatory.
A. P. Solonovich +2 more
doaj +1 more source
Revised coordinates of variable stars in Cassiopeia [PDF]
The identification of the variable stars published on IBVS 3573 has ben revised on the basis of the original (unpublished) finding charts. Cross check with the 2MASS catalog has been made to get more accurate coordinates and to confirm their nature from ...
R. Nesci, NESCI, R.
core +1 more source
Cataclysmic Variable Stars [PDF]
AbstractThe properties of cataclysmic variable outbursts are reviewed, and interpreted in terms of dynamical instabilities by the red component, and subsequent evolution of the white dwarf accretion disc subject to a mass transfer burst in the transfer stream.
openaire +1 more source
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
Semiregular Variable Stars [PDF]
19pages, in Ukrainian, 5 figures, 4 ...
openaire +2 more sources
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
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

