ASAS 160125-5150.3-the second galactic classical Cepheid with strong Blazhko effect

Repositorio Académico Institucional

Conocimiento Aplicado para la Innovación y el Desarrollo

dc.contributor.author	Kravtsov, Valery
dc.contributor.author	Berdnikov, L.N.
dc.contributor.author	Kniazev, A.Y.
dc.contributor.author	Dambis, A.K.
dc.date.accessioned	2020-09-14T15:25:11Z
dc.date.available	2020-09-14T15:25:11Z
dc.date.issued	2017
dc.identifier.citation	Astrophys Space Sci (2017) 362:105
dc.identifier.uri	https://hdl.handle.net/20.500.12740/16057
dc.description.abstract	In 2005–2014 we acquired a total of 135, 137 and 134 measurements in B-, V - and Ic-filters, respectively, for the 5-days Cepheid ASAS 160125-5150.3. Our observations showed variations of light amplitude, which allowed us to suspect the presence of the Blazhko effect. Combining our measurements with ASAS-3 data allowed us to determine the period of the Blazhko effect PBl = 1242d ± 10d , and now ASAS 160125-5150.3 is the second Galactic Cepheid (after V473 Lyr) with strong Blazhko effect pulsating in the first overtone
dc.language.iso	en
dc.rights	Atribución-SinDerivadas 3.0 Chile
dc.rights.uri	http://creativecommons.org/licenses/by-nd/3.0/cl/
dc.source.uri	DOI 10.1007/s10509-017-3088-x
dc.subject	VARIABLE STARS
dc.subject	PHOTOMETRY
dc.subject	CEPHEIDS
dc.subject	BLAZHKO EFFECT
dc.subject.other	EFECTO BLAZHKO
dc.title	ASAS 160125-5150.3-the second galactic classical Cepheid with strong Blazhko effect
dc.type	Artículo de Revista
dc.indice.citas	Science Citation Index Expanded
dc.relation.vrip	https://doi.org/10.1007/s10509-017-3088-x
dc.unidad	Física
dc.database	WoS-Scopus