Английская Википедия:HD 44120

Материал из Онлайн справочника
Перейти к навигацииПерейти к поиску

Шаблон:Short description Шаблон:Starbox begin Шаблон:Starbox observe Шаблон:Starbox character Шаблон:Starbox astrometry Шаблон:Starbox detail Шаблон:Starbox catalog Шаблон:Starbox reference Шаблон:Starbox end

HD 44120 is a wide binary star system in the southern constellation of Pictor. Although visible to the naked eye, it is a challenge to view having an apparent visual magnitude of 6.44.[1] The system is located at a distance of 118 light years from the Sun based on parallax, but it is drifting closer with a radial velocity of −2 km/s.[2] It has an absolute magnitude of 3.57.[1]

The primary member, designated component A of this system, is an F-type main-sequence star with a stellar classification of F9.5V.[3] It is a Sun-like star and has been considered a "hot" solar analog with a shallower convection zone than the Sun.[4] The estimated age of this star is about four billion years,[5] and it is spinning with a projected rotational velocity of 3.4 km/s.[6] It is chromospherically inactive.[7] The star has 1.2[5] times the mass of the Sun and 1.6[8] times the Sun's radius. It is radiating nearly three[8] times the luminosity of the Sun from its photosphere at an effective temperature of 6,005 K.[9]

The faint secondary companion, component C, is a magnitude 14.03 white dwarf star with a class of DB3.2,[10] indicating a helium-rich atmosphere. The object has an effective temperature of ~15,700 K with 67% of the Sun's mass but only 1.3% of the Sun's radius.[11] It has taken Шаблон:Val Myr for the white dwarf to have cooled to the current temperature. Prior to leaving the main sequence, this star is estimated to have had Шаблон:Val and thus was the system primary.[12] It has an angular separation of Шаблон:Val along a position angle of 301.6° from the current primary. The projected separation of this co-moving pair is Шаблон:Val. Their estimated orbit has a semimajor axis of Шаблон:Val and an orbital period of 51,100 years.[10]

A magnitude 7.61 visual companion, HD 44105, or component B, lies at an angular separation of Шаблон:Val along a position angle of 234° from component A, as of 2015. It was discovered as a double star by the Scottish astronomer James Dunlop and announced in 1829.[13] The parallax for this star indicates a distance of approximately Шаблон:Convert from the Sun.[14]

References

Шаблон:Reflist

Шаблон:Sky

Шаблон:Stars of Pictor

  1. 1,0 1,1 Ошибка цитирования Неверный тег <ref>; для сносок Anderson_Francis_2012 не указан текст
  2. Ошибка цитирования Неверный тег <ref>; для сносок Soubiran_et_al_2018 не указан текст
  3. Ошибка цитирования Неверный тег <ref>; для сносок Gray_et_al_2006 не указан текст
  4. Ошибка цитирования Неверный тег <ref>; для сносок González_Hernández_et_al_2012 не указан текст
  5. 5,0 5,1 Ошибка цитирования Неверный тег <ref>; для сносок Delgado_Mena_et_al_2019 не указан текст
  6. Ошибка цитирования Неверный тег <ref>; для сносок Delgado_Mena2_et_al_015 не указан текст
  7. Ошибка цитирования Неверный тег <ref>; для сносок Mason_et_al_1998 не указан текст
  8. 8,0 8,1 Ошибка цитирования Неверный тег <ref>; для сносок GaiaDR2 не указан текст
  9. Ошибка цитирования Неверный тег <ref>; для сносок Aguilera-Gómez_et_al_2018 не указан текст
  10. 10,0 10,1 Ошибка цитирования Неверный тег <ref>; для сносок Holberg_et_al_2013 не указан текст
  11. Ошибка цитирования Неверный тег <ref>; для сносок Bédard_et_al_2017 не указан текст
  12. Ошибка цитирования Неверный тег <ref>; для сносок Zhao_et_al_2012 не указан текст
  13. Ошибка цитирования Неверный тег <ref>; для сносок Mason_et_al_2014 не указан текст
  14. Ошибка цитирования Неверный тег <ref>; для сносок GaiaDR2B не указан текст