MX Андромеды

MX Андромеды
Звезда
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Наблюдательные данные
(Эпоха J2000.0)
Прямое восхождение 2ч 32м 3,10с[1]
Склонение +42° 08′ 30,48″[1]
Расстояние 18,41 кпк[2]
Видимая звёздная величина (V) 17,09[2]
Созвездие Андромеда
Астрометрия
Собственное движение
 • прямое восхождение 1,729 ± 0,189 mas/год[1]
 • склонение −1,379 ± 0,182 mas/год[1]
Параллакс (π) 0,0234 ± 0,1533 mas[1]
Спектральные характеристики
Переменность RR Лиры с асимметричной кривой блеска[вд][3][4][…]
Коды в каталогах
[KMW82] 23, 2MASS J02320310+4208304, Gaia DR2 338768431691725824, MX And, [SHM2017] J038.01291+42.14180, [DCD2013] CSS J023203.1+420829, [YWW2015] S527 2076 и TIC 203033464
Информация в базах данных
SIMBAD V* MX And
Логотип Викиданных Информация в Викиданных ?

MX Андромеды (лат. MX Andromedae) — одиночная переменная звезда[5][6] в созвездии Андромеды на расстоянии приблизительно 60045 световых лет (около 18410 парсеков) от Солнца. Видимая звёздная величина звезды — от +17,9m до +16,9m[7].

Характеристики

MX Андромеды — жёлто-белая пульсирующая переменная звезда типа RR Лиры (RRAB)[8][9][10] спектрального класса F5[7]. Эффективная температура — около 6751 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. ↑ 1 2 Drake A. J., Catelan M., Djorgovski S. G., Torrealba G., Graham M. J., Belokurov V., Koposov S. E., Mahabal A., Prieto J. L., Donalek C. et al. Probing the outer galactic halo with RR Lyrae from the Catalina surveys (англ.) // The Astrophysical Journal / E. Vishniac — IOP Publishing, 2013. — Vol. 763, Iss. 1. — P. 32. — ISSN 0004-637X; 1538-4357 — doi:10.1088/0004-637X/763/1/32 — arXiv:1211.2866
  3. ↑ Sesar B., Hernitschek N., Mitrović S., Ivezić Ž., Cohen J. G., Rix H., Bernard E. J., Grebel E. K., Martin N. F., Schlafly E. F. et al. Machine-learned Identification of RR Lyrae Stars from Sparse, Multi-band Data: The PS1 Sample (англ.) // The Astronomical Journal / J. G. III, E. Vishniac — New York City: IOP Publishing, AAS, University of Chicago Press, AIP, 2017. — Vol. 153, Iss. 5. — P. 204—219. — 16 p. — ISSN 0004-6256; 1538-3881 — doi:10.3847/1538-3881/AA661B — arXiv:1611.08596
  4. ↑ Yao X., Wang L., Wang X., Zhang T., Chen J., Yuan W., Mo J., Li W., Jin Z., Wu X. et al. Photometry of variable stars from the THU-NAOC transient survey. I. The first two years (англ.) // The Astronomical Journal / J. G. III, E. Vishniac — New York City: IOP Publishing, AAS, University of Chicago Press, AIP, 2015. — Vol. 150, Iss. 4. — 18 p. — ISSN 0004-6256; 1538-3881 — doi:10.1088/0004-6256/150/4/107 — arXiv:1507.08018
  5. ↑ Kinman T. D., Mahaffey C. T., Wirtanen C. A. An RR Lyrae survey with the lick astrograph. V. A survey of three fields at intermediate latitudes towards the Galactic Anticenter (англ.) // The Astronomical Journal / J. G. III, E. Vishniac — New York City: IOP Publishing, AAS, University of Chicago Press, AIP, 1982. — Vol. 87. — P. 314–352. — ISSN 0004-6256; 1538-3881 — doi:10.1086/113105
  6. ↑ Butler D., Kemper E., Kraft R. P., Suntzeff N. B. Metal abundances of RR Lyrae variables in selected galactic star fields. III. The Lick astrographic fields near the Galactic Anticenter (англ.) // The Astronomical Journal / J. G. III, E. Vishniac — New York City: IOP Publishing, AAS, University of Chicago Press, AIP, 1982. — Vol. 87. — P. 353–359. — ISSN 0004-6256; 1538-3881 — doi:10.1086/113106
  7. ↑ 1 2 MX 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 6 августа 2012 на Wayback Machine Accessed online 2020-12-27.
  8. ↑ Gavrilchenko T., Klein C. R., Bloom J. S., Richards J. W. A mid-infrared study of RR Lyrae stars with the Wide-field Infrared Survey Explorer all-sky data release (англ.) // Monthly Notices of the Royal Astronomical Society / D. Flower — OUP, 2014. — Vol. 441, Iss. 1. — P. 715–725. — ISSN 0035-8711; 1365-2966 — doi:10.1093/MNRAS/STU606 — arXiv:1312.4643
  9. ↑ Pier J. R., Saha A., Kinman T. D. Revised [Fe/H] and radial velocities for 28 distant RR Lyrae stars (англ.) // Information Bulletin on Variable Stars — Konkoly Observatory, 2003. — Vol. 5459. — P. 1. — ISSN 0374-0676; 1587-2440; 1587-6578
  10. ↑ Kholopov P. N., Samus N. N., Kazarovets E. V., Perova N. B. The 67th name-list of variable stars (англ.) // Information Bulletin on Variable Stars — Konkoly Observatory, 1985. — Vol. 2681. — P. 1–32. — ISSN 0374-0676; 1587-2440; 1587-6578

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