WOLF, Marek, Miloslav ZEJDA, Zdeněk MIKULÁŠEK, Jan JANÍK, Marek CHRASTINA, Marek SKARKA, Marek DROŹDŹ and Jerzy KREINER. NSVS 1065 3195 Ser: A New Low-Mass Binary. In Binaries - key to comprehension of the universe. volume 435. San Francisco: Astronomical society of the Pacific. p. 441-442. ISBN 978-1-58381-750-6. 2010.
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Basic information
Original name NSVS 1065 3195 Ser: A New Low-Mass Binary
Name in Czech NSVS 1065 3195 Ser: A New Low-Mass Binary
Authors WOLF, Marek (203 Czech Republic, guarantor), Miloslav ZEJDA (203 Czech Republic, belonging to the institution), Zdeněk MIKULÁŠEK (203 Czech Republic, belonging to the institution), Jan JANÍK (203 Czech Republic, belonging to the institution), Marek CHRASTINA (703 Slovakia, belonging to the institution), Marek SKARKA (203 Czech Republic, belonging to the institution), Marek DROŹDŹ (616 Poland) and Jerzy KREINER (616 Poland).
Edition volume 435. San Francisco, Binaries - key to comprehension of the universe, p. 441-442, 2 pp. 2010.
Publisher Astronomical society of the Pacific
Other information
Original language English
Type of outcome Proceedings paper
Field of Study 10308 Astronomy
Country of publisher United States of America
Confidentiality degree is not subject to a state or trade secret
Publication form printed version "print"
RIV identification code RIV/00216224:14310/10:00049404
Organization unit Faculty of Science
ISBN 978-1-58381-750-6
UT WoS 000289880000110
Keywords in English low mass binary; eclipsing binary; NSVS 1065 3195 star;
Tags AKb, rivok
Tags International impact, Reviewed
Changed by Changed by: RNDr. Jan Janík, Ph.D., učo 17241. Changed: 28/1/2013 10:07.
Abstract
In this paper we present a short study of newly discovered low mass eclipsing binary NSVS 1065 3195 based on our new photometric observations.Most of determinations of the fundamental parameters of low-mass stars using eclipsing binaries indicate a strong discrepancy between theory and observations. The measurements clearly indicate that the observed radii are generally larger than the predictions by stellar models. On the other hand the observed temperatures are lower than those predicted by the current models.
Links
GD205/08/H005, research and development projectName: Fyzika Slunce, hvězd a hvězdných soustav
Investor: Czech Science Foundation, Physics of Sun, stars, and stellar systems
IAA301630901, research and development projectName: Rozložení energie ve spektru horkých hvězd a jeho proměnnost
Investor: Academy of Sciences of the Czech Republic, Spectral energy distribution of hot stars and its variability
MEB050819, research and development projectName: Dvojhvězdnost - nástroj pro studium hvězdných charakteristik (Acronym: PLbinary)
Investor: Ministry of Education, Youth and Sports of the CR, Binarity - a tool for study of stellar characteristics, Programme KONTAKT - mobilities (MEB)
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