V362 Андромеды

V362 Андромеды
Звезда
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Наблюдательные данные
(Эпоха J2000.0)
Прямое восхождение 1ч 28м 7,00с[1]
Склонение +42° 28′ 1,06″[1]
Расстояние 916,0865 ± 43,5552 пк[1]
Видимая звёздная величина (V) 8,4 ± 0,01[2]
Созвездие Андромеда
Астрометрия
Лучевая скорость (Rv) −90,66 ± 0,49 км/с[1]
Собственное движение
 • прямое восхождение −6,782 ± 0,085 mas/год[1]
 • склонение −21,064 ± 0,092 mas/год[1]
Параллакс (π) 1,0916 ± 0,0519 mas[1]
Спектральные характеристики
Спектральный класс M0[3]
Показатель цвета
 • B−V 1,58
Коды в каталогах

AG+42 131, AGKR 1253, BD+41 278, GSC 02821-01909, HIC 6852, HIP 6852, IRAS 01251+4212, PPM 44018, SAO 37240, SKY# 2215, TYC 2821-1909-1, 2MASS J01280701+4228009, Gaia DR1 396396344363489152, Gaia DR2 396396348660465920, V362 And и TIC 191770718

Информация в базах данных
SIMBAD BD+41 278
Логотип Викиданных Информация в Викиданных ?

V362 Андромеды (лат. V362 Andromedae) — тройная звезда в созвездии Андромеды на расстоянии приблизительно 2988 световых лет (около 916 парсеков) от Солнца.

Пара первого и второго компонентов — двойная затменная переменная звезда (E:)[4][5]. Видимая звёздная величина звезды — от +8,55m до +8,42m[6]. Орбитальный период — около 18,519 суток[7].

Характеристики

Первый компонент — красный гигант спектрального класса M0[6][8][9][10]. Масса — около 1,762 солнечной, радиус — около 102,851 солнечных, светимость — около 1142,521 солнечных. Эффективная температура — около 3847 K[1].

Третий компонент — коричневый карлик. Масса — около 74,91 юпитерианских[11]. Удалён на 1,806 а.е.[11].

Примечания

  1. ↑ 1 2 3 4 5 6 7 8 Gaia Data Release 2 (англ.) / Data Processing and Analysis Consortium, European Space Agency — 2018.
  2. ↑ Høg E., Fabricius C., Makarov V. V., Urban S., Corbin T., Wycoff G., Bastian U., Schwekendiek P., Wicenec A. The Tycho-2 catalogue of the 2.5 million brightest stars (англ.) // Astronomy and Astrophysics / T. Forveille — EDP Sciences, 2000. — Vol. 355. — P. L27—L30. — ISSN 0004-6361; 0365-0138; 1432-0746; 1286-4846
  3. ↑ SIMBAD Astronomical Database
  4. ↑ Avvakumova E. A., Malkov O. Y., Kniazev A. Y. Eclipsing variables: Catalogue and classification (англ.) // Astronomische Nachrichten — Wiley, 2013. — Vol. 334, Iss. 8. — P. 860—865. — ISSN 0004-6337; 1521-3994 — doi:10.1002/ASNA.201311942
  5. ↑ Kazarovets E. V., Samus N. N., Durlevich O. V., Frolov M. S., Antipin S. V., Kireeva N. N., Pastukhova E. N. The 74th special name-list of variable stars (англ.) // Information Bulletin on Variable Stars — Konkoly Observatory, 1999. — Vol. 4659. — P. 1–27. — ISSN 0374-0676; 1587-2440; 1587-6578
  6. ↑ 1 2 V362 And, database entry, Combined General Catalog of Variable Stars (GCVS5.1, 2017 Ed.), N. N. Samus, O. V. Durlevich, et al., CDS ID II/250 Архивная копия от 1 июля 2015 на Wayback Machine Accessed online 2021-01-04.
  7. ↑ N. N. Samus’, Kazarovets E. V., Durlevich O. V., Kireeva N. N., Pastukhova E. N. General catalogue of variable stars: Version GCVS 5.1 (англ.) // Astronomy Reports / D. Bisikalo — MAIK Nauka/Interperiodica, Springer Science+Business Media, 2017. — Vol. 61, Iss. 1. — P. 80–88. — ISSN 1063-7729; 1562-6881; 0004-6299 — doi:10.1134/S1063772917010085
  8. ↑ Roeser S., Bastian U. PPM (Positions and Proper Motions) North Star Catalogue (англ.) // Astronomy and Astrophysics / T. Forveille — EDP Sciences, 1988. — Vol. 74. — P. 449. — ISSN 0004-6361; 0365-0138; 1432-0746; 1286-4846
  9. ↑ Cruzalèbes P., Petrov R. G., Robbe-Dubois S., Varga J., Burtscher L., Allouche F., Berio P., Hofmann, K. -H., Hron J., Jaffe W. et al. A catalogue of stellar diameters and fluxes for mid-infrared interferometry (англ.) // Monthly Notices of the Royal Astronomical Society / D. Flower — OUP, 2019. — Vol. 490, Iss. 3. — P. 3158—3176. — ISSN 0035-8711; 1365-2966 — doi:10.1093/MNRAS/STZ2803 — arXiv:1910.00542
  10. ↑ Koen C., Eyer L. New periodic variables from the Hipparcos epoch photometry (англ.) // Monthly Notices of the Royal Astronomical Society / D. Flower — OUP, 2002. — Vol. 331, Iss. 1. — P. 45–59. — 15 p. — ISSN 0035-8711; 1365-2966 — doi:10.1046/J.1365-8711.2002.05150.X — arXiv:astro-ph/0112194
  11. ↑ 1 2 Kervella P., Arenou F., Mignard F., Thévenin F. Stellar and substellar companions of nearby stars from Gaia DR2. Binarity from proper motion anomaly (англ.) // Astronomy and Astrophysics / T. Forveille — EDP Sciences, 2019. — Vol. 623. — P. 72–72. — 23 p. — ISSN 0004-6361; 0365-0138; 1432-0746; 1286-4846 — doi:10.1051/0004-6361/201834371 — arXiv:1811.08902

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