Results 11 to 20 of about 3,822 (305)

Classification of variable stars in the WFCAM Transit Survey

EPJ Web of Conferences, 2013
The WFCAM Transit Survey is a photometric survey in the near-infrared and aims at finding Earth-like planets transiting M-dwarf stars. As a by-product of the survey, a variety of variable stars has been detected.
Moya Andrés, Barrado David, Sarro Luis M., Stoev Hristo   +3 more
doaj   +2 more sources

A Classification Catalog of Periodic Variable Stars for LAMOST DR9 Based on Machine Learning

The Astrophysical Journal Supplement Series
Identifying and classifying variable stars is essential to time-domain astronomy. The Large Area Multi-Object Fiber Optic Spectroscopic Telescope (LAMOST) acquired a large amount of spectral data.
Peiyun Qiao, Tingting Xu, Feng Wang, Ying Mei, Hui Deng, Lei Tan, Chao Liu   +6 more
doaj   +2 more sources

Search for variable stars in the young open cluster Stock 18 [PDF]

EPJ Web of Conferences, 2017
We have carried out multi-epoch deep I band photometry of the open cluster Stock 18 to search for variable stars in star forming regions. In the present study, we report identification of 28 periodic and 165 non-periodic variables stars.
Sinha Tirthendu, Sharma Saurabh, Pandey Rakesh, Pandey A.K.   +3 more
doaj   +2 more sources

Automated classification of periodic variable stars{Improved methodology for the automated classification of periodic variable stars} [PDF]

, 2011
11 pages, 6 figures Accepted for publication in ...
Blomme, J., Sarro, L. M., O'Donovan, F. T., Debosscher, J., Brown, T., Lopez, M., Dubath, P., Rimoldini, L., Charbonneau, D., Dunham, E., Mandushev, G., Ciardi, D. R., De Ridder, J., Aerts, C.   +13 more
openaire   +3 more sources

Searching for Anomalies in the ZTF Catalog of Periodic Variable Stars

, 2021
Periodic variables illuminate the physical processes of stars throughout their lifetime. Wide-field surveys continue to increase our discovery rates of periodic variable stars.
Drout, Maria R., Villar, V. Ashley, Renzo, Mathieu, Chan, H. S., Ho, Shirley, O'Grady, Anna J. G., Cheung, S. H.   +6 more
core   +1 more source

Classification of The Zwicky Transient Facility Catalog of Periodic Variable Stars

, 2021
This data release contains 730,184 periodic transients with the new class labels in a csv file and the cross-match results of periodic variable stars (PVSs) in the ZTF CPVS with the SIMBAD catalog.
Villar, V. Ashley, Chan, Ho-Sang, Ho, Shirley, Cheung, Siu Hei   +3 more
core   +1 more source

Variable stars of short period.

The Astrophysical Journal, 1880
Reprinted from the Proceedings of the American academy of arts and sciences, vol. XVI. ; Mode of access: Internet.
openaire   +3 more sources

Detecting Short Period Variable Stars with Gaia [PDF]

AIP Conference Proceedings, 2009
We analyzed the frequency domain of time series of simulated ZZ Ceti light-curves to investigate the detectability and period recovery performance of short period variables (periods < 2 hours) for the Gaia mission. In our analysis, first we used a non-linear ZZ Ceti light-curves simulator code to simulate the variability of ZZ Ceti stars (we assumed
Mihaly Varadi, Laurent Eyer, Stefan Jordan, Nami Mowlavi, Detlev Koester, Joyce Ann Guzik, Paul A. Bradley   +6 more
openaire   +2 more sources

Short-period variability in Be stars [PDF]

Monthly Notices of the Royal Astronomical Society, 1990
Summary A highly significant correlation is found between the projected rotational velocities and the photometric periods of Be stars. We show that this correlation may be readily understood if the photometric period is equated with the rotational period.
openaire   +1 more source

The Periods of Cataclysmic Variable Stars [PDF]

International Astronomical Union Colloquium, 1983
To understand the structure and evolution of the cataclysmic variables, we will need accurate values for their masses, dimensions, mass transfer rates, and other physical properties. Unfortunately, despite an abundance of observational data on these systems, there is a severe dearth of reliable, quantitative information about their fundamental physical
openaire   +1 more source