CzeV1731: The unique doubly eclipsing quadruple system

J 2020

CzeV1731: The unique doubly eclipsing quadruple system

ZASCHE, P.; Z. HENZL; H. LEHMANN; J. PEPPER; B. P. POWELL et. al.

Basic information

Original name

CzeV1731: The unique doubly eclipsing quadruple system

Authors

ZASCHE, P.; Z. HENZL; H. LEHMANN; J. PEPPER; B. P. POWELL; V. B. KOSTOV; T. BARCLAY; M. WOLF; Hana KUČÁKOVÁ (203 Czech Republic, belonging to the institution); R. UHLAR; M. MASEK; S. PALAFOUTA; K. GAZEAS; K. G. STASSUN; B. S. GAUDI; J. E RODRIGUEZ and D. J. STEVENS

Edition

Astronomy & Astrophysics, FR - Francouzská republika, 2020, 0004-6361

Other information

Language

English

Type of outcome

Article in a journal

Field of Study

10308 Astronomy

Country of publisher

France

Confidentiality degree

is not subject to a state or trade secret

References:

URL

Impact factor

Impact factor: 5.803

RIV identification code

RIV/47813059:19630/20:A0000065

Organization unit

Institute of physics in Opava

DOI

https://doi.org/10.1051/0004-6361/202038656

UT WoS

000581811000001

EID Scopus

2-s2.0-85093928172

Keywords in English

binaries: eclipsing; binaries: spectroscopic; stars: fundamental parameters

Abstract

In the original language

We report the discovery of the relatively bright (V=10.5 mag), doubly eclipsing 2+2 quadruple system CzeV1731. This is the third known system of its kind, in which the masses are determined for all four stars and both the inner and outer orbits are characterized. The inner eclipsing binaries are well-detached systems moving on circular orbits: pair A with period P-A=4.10843 d and pair B with P-B=4.67552 d. The inner binaries contain very similar components (q approximate to 1.0), making the whole system a so-called double twin. The stars in pair B have slightly larger luminosities and masses and pair A shows deeper eclipses. All four components are main-sequence stars of F/G spectral type. The mutual orbit of the two pairs around the system barycenter has a period of about 34 yr and an eccentricity of about 0.38. However, further observations are needed to reveal the overall architecture of the whole system, including the mutual inclinations of all orbits. This is a promising target for interferometry to detect the double at about 59 mas and Delta M-bol< 1 mag.

Cite

ZASCHE, P.; Z. HENZL; H. LEHMANN; J. PEPPER; B. P. POWELL; V. B. KOSTOV; T. BARCLAY; M. WOLF; Hana KUČÁKOVÁ; R. UHLAR; M. MASEK; S. PALAFOUTA; K. GAZEAS; K. G. STASSUN; B. S. GAUDI; J. E RODRIGUEZ and D. J. STEVENS. CzeV1731: The unique doubly eclipsing quadruple system. Astronomy & Astrophysics. FR - Francouzská republika, 2020, vol. 642, October, p. "A63-1"-"A63-5", 5 pp. ISSN 0004-6361. Available from: https://doi.org/10.1051/0004-6361/202038656.

@article{49287,
   author = {Zasche, P. and Henzl, Z. and Lehmann, H. and Pepper, J. and Powell, B. P. and Kostov, V. B. and Barclay, T. and Wolf, M. and Kučáková, Hana and Uhlar, R. and Masek, M. and Palafouta, S. and Gazeas, K. and Stassun, K. G. and Gaudi, B. S. and Rodriguez, J. E and Stevens, D. J.},
   article_location = {FR - Francouzská republika},
   article_number = {October},
   doi = {https://doi.org/10.1051/0004-6361/202038656},
   keywords = {binaries: eclipsing; binaries: spectroscopic; stars: fundamental parameters},
   language = {eng},
   issn = {0004-6361},
   journal = {Astronomy & Astrophysics},
   title = {CzeV1731: The unique doubly eclipsing quadruple system},
   url = {https://www.aanda.org/articles/aa/abs/2020/10/aa38656-20/aa38656-20.html},
   volume = {642},
   year = {2020}
}

TY  - JOUR
ID  - 49287
AU  - Zasche, P. - Henzl, Z. - Lehmann, H. - Pepper, J. - Powell, B. P. - Kostov, V. B. - Barclay, T. - Wolf, M. - Kučáková, Hana - Uhlar, R. - Masek, M. - Palafouta, S. - Gazeas, K. - Stassun, K. G. - Gaudi, B. S. - Rodriguez, J. E - Stevens, D. J.
PY  - 2020
TI  - CzeV1731: The unique doubly eclipsing quadruple system
JF  - Astronomy & Astrophysics
VL  - 642
IS  - October
SP  - "A63-1"-"A63-5"
EP  - "A63-1"-"A63-5"
SN  - 00046361
KW  - binaries: eclipsing
KW  - binaries: spectroscopic
KW  - stars: fundamental parameters
UR  - https://www.aanda.org/articles/aa/abs/2020/10/aa38656-20/aa38656-20.html
N2  - We report the discovery of the relatively bright (V=10.5 mag), doubly eclipsing 2+2 quadruple system CzeV1731. This is the third known system of its kind, in which the masses are determined for all four stars and both the inner and outer orbits are characterized. The inner eclipsing binaries are well-detached systems moving on circular orbits: pair A with period P-A=4.10843 d and pair B with P-B=4.67552 d. The inner binaries contain very similar components (q approximate to 1.0), making the whole system a so-called double twin. The stars in pair B have slightly larger luminosities and masses and pair A shows deeper eclipses. All four components are main-sequence stars of F/G spectral type. The mutual orbit of the two pairs around the system barycenter has a period of about 34 yr and an eccentricity of about 0.38. However, further observations are needed to reveal the overall architecture of the whole system, including the mutual inclinations of all orbits. This is a promising target for interferometry to detect the double at about 59 mas and Delta M-bol< 1 mag.
ER  -

ZASCHE, P.; Z. HENZL; H. LEHMANN; J. PEPPER; B. P. POWELL; V. B. KOSTOV; T. BARCLAY; M. WOLF; Hana KUČÁKOVÁ; R. UHLAR; M. MASEK; S. PALAFOUTA; K. GAZEAS; K. G. STASSUN; B. S. GAUDI; J. E RODRIGUEZ and D. J. STEVENS. CzeV1731: The unique doubly eclipsing quadruple system. \textit{Astronomy \&{} Astrophysics}. FR - Francouzská republika, 2020, vol.~642, October, p.~''A63-1''-''A63-5'', 5 pp. ISSN~0004-6361. Available from: https://doi.org/10.1051/0004-6361/202038656.

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