A photometric study of NSVS 7453183: a probable quadruple system with long-term surface activity
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F23%3A00571136" target="_blank" >RIV/67985815:_____/23:00571136 - isvavai.cz</a>
Alternative codes found
RIV/00098639:_____/23:N0000001 RIV/00216224:14310/23:00130441 RIV/47813059:19630/23:A0000318 RIV/00216208:11320/23:10475179
Result on the web
<a href="https://hdl.handle.net/11104/0342428" target="_blank" >https://hdl.handle.net/11104/0342428</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1093/mnras/stad053" target="_blank" >10.1093/mnras/stad053</a>
Alternative languages
Result language
angličtina
Original language name
A photometric study of NSVS 7453183: a probable quadruple system with long-term surface activity
Original language description
The VRC light curves were regularly measured for the eclipsing binary NSVS 7453183 as a part of our long-term observational project for studying of low-mass eclipsing binaries with a short orbital period and surface activity. The TESS light curve solution in phoebe results to the detached configuration, where the temperature of primary component was adopted to T-1 = 4300K according to the SED approximation. It gives us T-2 = 4080 +/- 100K for the secondary component. The spectral type of the primary component was estimated to be K6, and the photometric mass ratio was derived q = 0.86. We confirm presence of the third body in this system, a stellar companion with a minimal mass 0.33M(circle dot) orbiting the eclipsing pair with a short period about 425 days, and propose the next, fourth body with a longer orbiting period of about 12 years, probably a brown dwarf with the minimal mass of 50M(Jup). The hierarchical structure ((1+1)+1) + 1 of this quadruple system is assumed. Characteristics and temporal variations of the dark region on the surface of the primary component were estimated. The average migration speed of about 10 degrees per month was found during years 2020-2022.
Czech name
—
Czech description
—
Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
—
OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
—
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2023
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Monthly Notices of the Royal Astronomical Society
ISSN
0035-8711
e-ISSN
1365-2966
Volume of the periodical
520
Issue of the periodical within the volume
1
Country of publishing house
US - UNITED STATES
Number of pages
11
Pages from-to
353-363
UT code for WoS article
000928268000005
EID of the result in the Scopus database
2-s2.0-85161604803