Английская Википедия:EZ Canis Majoris

Материал из Онлайн справочника
Перейти к навигацииПерейти к поиску

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

EZ Canis Majoris (abbreviated to EZ CMa, also designated as WR 6) is binary system in the constellation of Canis Major. The primary is a Wolf-Rayet star and it is one of the ten brightest Wolf-Rayet stars, brighter than apparent magnitude 7.[1]

Binary system

Файл:Sh2-308.jpg
Detail of one edge of the bubble blown by EZ CMa. EZ CMa is off frame to the left (east).

EZ CMa has an apparent visual magnitude which varies between 6.71 and 6.95 over a period of 3.766 days, along with changes in the spectrum.[2] It has been proposed that it could be a binary star, with a neutron star as companion that would complete an orbit around the Wolf-Rayet with that period, being the cause of those variations. The General Catalogue of Variable Stars lists it as a possible cataclysmic variable on this basis. It has been argued that the companion does not exist and spectral variations are caused by activity on the star's surface.[2]

Файл:EZCMaLightCurve.png
A light curve for EZ Canis Majoris, plotted from TESS data[3]

Observations of the light variations over a four-month period from late 2015 to early 2016 confirmed the clear Шаблон:Val variations. This was interpreted as a Шаблон:Val orbital period with rapid apsidal precession completing a full rotation in about 100 days. The orbit is inclined at around 60–74 degrees and there are two eclipses during each orbit.[4]

Wolf Rayet star and nebula

The spectral type of WN4 indicates an extremely hot star, and this leads to a very high luminosity, mostly emitted as ultraviolet radiation. The spectrum shows a star entirely devoid of hydrogen at the surface.[5]

EZ CMa is surrounded by a faint bubble nebula, a small HII region blown by stellar winds up to 1,700 km/s and ionised by the intense UV radiation. This is catalogued as Sharpless Sh2-308, or just S308.[6] It is likely to be a member of the very scattered open cluster Collinder 121, found around the orange supergiant ο1 CMa.

References

Шаблон:Reflist

External links

Шаблон:Stars of Canis Major

Партнерские ресурсы
Криптовалюты
Магазины
Хостинг
Разное

  1. ↑ Шаблон:Cite journal
  2. ↑ 2,0 2,1 Шаблон:Cite journal
  3. ↑ Ошибка цитирования Неверный тег <ref>; для сносок MAST не указан текст
  4. ↑ Ошибка цитирования Неверный тег <ref>; для сносок schmutz не указан текст
  5. ↑ Ошибка цитирования Неверный тег <ref>; для сносок wn не указан текст
  6. ↑ Шаблон:Cite journal
Источник — http://wikihandbk.com/ruwiki/index.php?title=Английская_Википедия:EZ_Canis_Majoris&oldid=14425296