V416 Андромеды

V416 Андромеды
Звезда
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Наблюдательные данные
(Эпоха J2000.0)
Прямое восхождение 1ч 10м 30,43с[1]
Склонение +45° 06′ 11,57″[1]
Созвездие Андромеда
Астрометрия
Собственное движение
 • прямое восхождение 1,574 ± 0,36 mas/год[1]
 • склонение −3,083 ± 0,361 mas/год[1]
Параллакс (π) 0,0753 ± 0,1975 mas[1]
Спектральные характеристики
Переменность мирида[2]
Коды в каталогах
2MASS J01103043+4506115, GSC 03264-00924, IRAS 01076+4450, Gaia DR2 376816623550472960, V416 And, WISE J011030.44+450613.3, AAVSO 0104+44, LD 338, [WWV2004] J0110303+450610 и TIC 196694724
Информация в базах данных
SIMBAD V* V416 And
Логотип Викиданных Информация в Викиданных ?

V416 Андромеды (лат. V416 Andromedae) — одиночная переменная звезда[3][4][5] в созвездии Андромеды на расстоянии (вычисленном из значения параллакса) приблизительно 43314 световых лет (около 13280 парсеков) от Солнца. Видимая звёздная величина звезды — от менее +14,7m до +11,7m[6].

Характеристики

V416 Андромеды — красная пульсирующая переменная звезда, мирида (M)[6][7][8] спектрального класса M. Эффективная температура — около 3293 K[1].

Примечания

  1. 1 2 3 4 5 6 Gaia Data Release 2 (англ.) / Data Processing and Analysis Consortium, European Space Agency — 2018.
  2. Woźniak P. R., Williams S. J., Vestrand W. T., Gupta V. Identifying red variables in the Northern Sky Variability Survey (англ.) // The Astronomical Journal / J. G. III, E. Vishniac — New York City: IOP Publishing, AAS, University of Chicago Press, AIP, 2004. — Vol. 128, Iss. 6. — P. 2965–2976. — ISSN 0004-6256; 1538-3881doi:10.1086/425526
  3. Heinze A. N., Tonry J. L., Denneau L., Stalder B., Rest A., Smith K. W., Smartt S. J., Weiland H. A First Catalog of Variable Stars Measured by the Asteroid Terrestrial-impact Last Alert System (ATLAS) (англ.) // The Astronomical Journal / J. G. III, E. Vishniac — New York City: IOP Publishing, AAS, University of Chicago Press, AIP, 2018. — Vol. 156, Iss. 5. — P. 241. — ISSN 0004-6256; 1538-3881doi:10.3847/1538-3881/AAE47FarXiv:1804.02132
  4. Deguchi S., Sakamoto T., Hasegawa T. Kinematics of red variables in the Solar neighborhood. I.Basic data obtained by an SiO maser survey (англ.) // Publications of the Astronomical Society of JapanOUP, Astronomical Society of Japan, 2012. — Vol. 64, Iss. 1. — 39 p. — ISSN 0004-6264; 2053-051Xdoi:10.1093/PASJ/64.1.4arXiv:1108.4491
  5. Kazarovets E. V., Samus N. N., Durlevich O. V. The 76th name-list of variable stars (англ.) // Information Bulletin on Variable StarsKonkoly Observatory, 2001. — Vol. 5135. — P. 1. — ISSN 0374-0676; 1587-2440; 1587-6578
  6. 1 2 V416 And Архивная копия от 26 июля 2020 на Wayback Machine, 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 2021-01-18.
  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. BisikaloMAIK Nauka/Interperiodica, Springer Science+Business Media, 2017. — Vol. 61, Iss. 1. — P. 80–88. — ISSN 1063-7729; 1562-6881; 0004-6299doi:10.1134/S1063772917010085
  8. Dahlmark L. New variable stars in Andromeda and Cassiopeia (англ.) // Information Bulletin on Variable StarsKonkoly Observatory, 1999. — Vol. 4734. — P. 1–4. — ISSN 0374-0676; 1587-2440; 1587-6578

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