Three new 2+2 quadruple systems with changing inclination

J 2025

Three new 2+2 quadruple systems with changing inclination

ZASCHE, P.; Z. HENZL; M. MASEK; J. KARA; Hana KUČÁKOVÁ et al.

Základní údaje

Originální název

Three new 2+2 quadruple systems with changing inclination

Autoři

ZASCHE, P.; Z. HENZL; M. MASEK; J. KARA; Hana KUČÁKOVÁ; J. MERC a R. UHLAR

Vydání

Monthly Notices of the Royal Astronomical Society, US - Spojené státy americké, 2025, 0035-8711

Další údaje

Jazyk

angličtina

Typ výsledku

Článek v odborném periodiku

Obor

10308 Astronomy

Stát vydavatele

Velká Británie a Severní Irsko

Utajení

není předmětem státního či obchodního tajemství

Odkazy

URL

Impakt faktor

Impact factor: 4.800 v roce 2024

Organizační jednotka

Fyzikální ústav v Opavě

DOI

https://doi.org/10.1093/mnras/staf495

UT WoS

001468670700001

EID Scopus

2-s2.0-105002843288

Klíčová slova anglicky

binaries: close;binaries: eclipsing

Štítky

RIV26, UF

Příznaky

Mezinárodní význam, Recenzováno

Změněno: 28. 1. 2026 12:07, Mgr. Pavlína Jalůvková

Anotace

V originále

We present a unique discovery of three new detected systems showing two different phenomena together. These are 2+2 quadruple stellar systems showing two eclipsing binaries as the inner pairs. And besides that, these systems were also found to exhibit the precession of the inner orbits causing the inclination changes manifesting themselves through the eclipse depth variations. We are not aware of any similar known system on the sky nowadays, hence our discovery is really unique. In particular these systems are: CzeV4315 = HD 228777 (periods 6.7391 and 0.91932 d, inclination change of pair B of about 1.4 yr-1); ASASSN-V J075203.23-323102.7 = GDS_J0752031-323102 (8.86916 d + 2.6817 d, inclination change of pair B of about 1.03 yr-1, now only ellipsoidal variations); ASASSN-V J105824.33-611347.6 = TIC 465899856 (2.3304 d + 13.0033 d, inclination change of pair B, now undetectable). These systems provide us unique insight into the quadruple-star dynamics, including the orbit-orbit interaction, Kozai-Lidov cycles, and testing the stellar formation theories of these higher order multiples.

Citovat

ZASCHE, P.; Z. HENZL; M. MASEK; J. KARA; Hana KUČÁKOVÁ; J. MERC a R. UHLAR. Three new 2+2 quadruple systems with changing inclination. Monthly Notices of the Royal Astronomical Society. US - Spojené státy americké, 2025, roč. 539, č. 2, s. 1015-1023. ISSN 0035-8711. Dostupné z: https://doi.org/10.1093/mnras/staf495.

@article{90422,
   author = {Zasche, P. and Henzl, Z. and Masek, M. and Kara, J. and Kučáková, Hana and Merc, J. and Uhlar, R.},
   article_location = {US - Spojené státy americké},
   article_number = {2},
   doi = {https://doi.org/10.1093/mnras/staf495},
   keywords = {binaries: close;binaries: eclipsing},
   language = {eng},
   issn = {0035-8711},
   journal = {Monthly Notices of the Royal Astronomical Society},
   title = {Three new 2+2 quadruple systems with changing inclination},
   url = {https://watermark02.silverchair.com/staf495.pdf?token=AQECAHi208BE49Ooan9kkhW_Ercy7Dm3ZL_9Cf3qfKAc485ysgAAA3gwggN0BgkqhkiG9w0BBwagggNlMIIDYQIBADCCA1oGCSqGSIb3DQEHATAeBglghkgBZQMEAS4wEQQMU3fcP1YPg-i6OGy5AgEQgIIDK30moOCyeqZWPsabczGJAZV0HBngMmT1nKN1uujJzgbl},
   volume = {539},
   year = {2025}
}

TY  - JOUR
ID  - 90422
AU  - Zasche, P. - Henzl, Z. - Masek, M. - Kara, J. - Kučáková, Hana - Merc, J. - Uhlar, R.
PY  - 2025
TI  - Three new 2+2 quadruple systems with changing inclination
JF  - Monthly Notices of the Royal Astronomical Society
VL  - 539
IS  - 2
SP  - 1015-1023
EP  - 1015-1023
SN  - 00358711
KW  - binaries: close;binaries: eclipsing
UR  - https://watermark02.silverchair.com/staf495.pdf?token=AQECAHi208BE49Ooan9kkhW_Ercy7Dm3ZL_9Cf3qfKAc485ysgAAA3gwggN0BgkqhkiG9w0BBwagggNlMIIDYQIBADCCA1oGCSqGSIb3DQEHATAeBglghkgBZQMEAS4wEQQMU3fcP1YPg-i6OGy5AgEQgIIDK30moOCyeqZWPsabczGJAZV0HBngMmT1nKN1uujJzgbl
N2  - We present a unique discovery of three new detected systems showing two different phenomena together. These are 2+2 quadruple stellar systems showing two eclipsing binaries as the inner pairs. And besides that, these systems were also found to exhibit the precession of the inner orbits causing the inclination changes manifesting themselves through the eclipse depth variations. We are not aware of any similar known system on the sky nowadays, hence our discovery is really unique. In particular these systems are: CzeV4315 = HD 228777 (periods 6.7391 and 0.91932 d, inclination change of pair B of about 1.4 yr-1); ASASSN-V J075203.23-323102.7 = GDS_J0752031-323102 (8.86916 d + 2.6817 d, inclination change of pair B of about 1.03 yr-1, now only ellipsoidal variations); ASASSN-V J105824.33-611347.6 = TIC 465899856 (2.3304 d + 13.0033 d, inclination change of pair B, now undetectable). These systems provide us unique insight into the quadruple-star dynamics, including the orbit-orbit interaction, Kozai-Lidov cycles, and testing the stellar formation theories of these higher order multiples.
ER  -

ZASCHE, P.; Z. HENZL; M. MASEK; J. KARA; Hana KUČÁKOVÁ; J. MERC a R. UHLAR. Three new 2+2 quadruple systems with changing inclination. \textit{Monthly Notices of the Royal Astronomical Society}. US - Spojené státy americké, 2025, roč.~539, č.~2, s.~1015-1023. ISSN~0035-8711. Dostupné z: https://doi.org/10.1093/mnras/staf495.

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