Results 1 to 10 of about 51,534 (310)
Classification of Periodic Variable Stars from TESS
The number of known periodic variable stars has increased rapidly in recent years. As an all-sky transit survey, the Transiting Exoplanet Survey Satellite (TESS) plays an important role in detecting low-amplitude variable stars.
Xinyi Gao +3 more
doaj +2 more sources
Variable stars are those whose brightness changes over time. Astronomers (amateurs and professionals alike) have played an integral role in making variable star observations, resulting in significant databases that are used to study these objects.
Arndt, Martina
core +5 more sources
New triple-mode high-amplitude Delta Scuti variables
I present a detection of four new triple-mode high-amplitude Delta Scuti variables, pulsating in the fundamental, first, and second overtone modes. This is a new addition to the ten known cases in the Galaxy.
Khruslov Anton V.
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Streaming classification of variable stars [PDF]
ABSTRACTIn the last years, automatic classification of variable stars has received substantial attention. Using machine learning techniques for this task has proven to be quite useful. Typically, machine learning classifiers used for this task require to have a fixed training set, and the training process is performed offline.
Zorich, L +2 more
openaire +3 more sources
Most Rotational Variables Dominated by a Single Bright Feature Are α 2 CVn Stars
We previously reported a rare class of variable star light curves isolated from a sample of 4.7 million candidate variables from the ATLAS survey. Dubbed “UCBH” light curves, they have broad minima and narrow, symmetrical maxima, with typical periods of ...
A. N. Heinze +2 more
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Future of the General Catalogue of Variable Stars from the Experience of Recent Name-lists
We briefly outline the history of the General Catalogue of Variable Stars (GCVS) and the New Catalogue of Suspected Variable Stars (NSV catalogue). Recently, we have completed a revision of the NSV catalogue.
Samus Nikolay N. +5 more
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NEW VARIABLE STAR IN THE ORION CONSTELLATION
New variable star with α = 05° 57m22s, δ = +20°15.5' (1950) was discovered with elements JD Max=2436999.28 + 0.2343973 E, range 15.6- 16.2m (pg) and asymmetry M-m=0.26.
I. S. Brjukhanov, V. P. Goranskij
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New periodic variable stars coincident with ROSAT sources discovered using SuperWASP [PDF]
We present optical lightcurves of 428 periodic variable stars coincident with ROSAT X-ray sources, detected using the first run of the SuperWASP photometric survey. Only 68 of these were previously recognised as periodic variables.
West, Richard G. +75 more
core +1 more source
The measurements of brightness of the star IRAS 17583+5150 discovered using the Odessa observatory negatives are discussed in the article. The proposed types of these stars are IRAS 17583+5150 -- type SRB (SRC).
A. P. Solonovich, I. S. Bryukhanov
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OBSERVATIONS OF VARIABLE STARS WITH SMALL TELESCOPES
No ...
I. S. Bryukhanov
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