翻訳と辞書
Words near each other
・ Qırx Çıraq
・ Qırxbulaq
・ Qırxıncı
・ Qırılı
・ Quỳnh Lưu District
・ Quỳnh Lưu Uprising
・ Quỳnh Nhai District
・ Quỳnh Phụ District
・ Quỳnh Sơn
・ Quỳnh Văn culture
・ Qu’Appelle Valley Hockey League
・ Qu’est-ce Pour Nous
・ Qu’nyido
・ Qu’og
・ QV
QV Normae
・ QV Telescopii
・ QV.1
・ QV44
・ QV60
・ QV66
・ QV68
・ QV71
・ QV75
・ QV80
・ Qvale
・ Qvale Mangusta
・ Qvareli Municipality
・ Qvarforth
・ QVC


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QV Normae : ウィキペディア英語版
QV Normae


QV Normae, also known as Norma X-2, is a high mass X-ray binary star system in the constellation Norma. It varies between apparent magnitudes of 16.19 and 16.31.
The X-ray source was first identified in the early 1970s.〔 The nature of the system was discovered in 1978 by astronomers who aligned a visual source of a reddened hot blue-white star with the X-ray source 4U 1538 - 52. The components are a blue-white supergiant estimated to have a mass around 20 times that of our Sun and a neutron star initially estimated at around 1.4 solar masses, later revised to 0.8 solar masses. The stellar wind from the more massive star is drawn to the magnetic poles of neutron star, forming an accretion column and producing X-rays. The system has been estimated to lie anywhere from 4500 to 6500 parsecs (15,000-20,000 light-years) from Earth.

== References ==



抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
ウィキペディアで「QV Normae」の詳細全文を読む



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