NSVS 1065 3195 Ser: A New Low-Mass Binary

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, 2010, p. 441-442. ISBN 978-1-58381-750-6.

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

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Other information

Language

English

Type of outcome

Stať ve sborníku

Field of Study

10308 Astronomy

Country of publisher

United States of America

Confidentiality degree

není předmětem státního či obchodního tajemství

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

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Abstract

V originále

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.

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Links

GD205/08/H005, research and development project	Name: Fyzika Slunce, hvězd a hvězdných soustav Investor: Czech Science Foundation, Physics of Sun, stars, and stellar systems
IAA301630901, research and development project	Name: 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 project	Name: 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)