About: RCW 103 — revisiting a cooling neutron star

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Attributs	Valeurs
type	work Article
Is Part Of	http://hub.abes.fr/oup/periodical/mnras/1998/volume_298/issue_1/w
Subject	radiative transfer stars: magnetic fields stars: neutron Letters X-rays: stars
Title	RCW 103 — revisiting a cooling neutron star
has manifestation of work	http://hub.abes.fr/oup/periodical/mnras/1998/volume_298/issue_1/101046j13658711199801853x/m/print http://hub.abes.fr/oup/periodical/mnras/1998/volume_298/issue_1/101046j13658711199801853x/m/web
related by	http://hub.abes.fr/oup/periodical/mnras/1998/volume_298/issue_1/101046j13658711199801853x/authorship/2 http://hub.abes.fr/oup/periodical/mnras/1998/volume_298/issue_1/101046j13658711199801853x/authorship/1
Author	Hernquist Lars Heyl Jeremy S.
Abstract	Abstract. Recent observations of the compact source embedded within the supernova remnant RCW 103 rekindle interest in the origin of this object's emission. We contrast several models in which neutron-star cooling powers RCW 103. Specifically, either the presence of an accreted envelope or a sufficiently intense magnetic field can account for the X-Ray emission from this object.
article type	research-article
is part of this journal	Monthly Notices of the Royal Astronomical Society

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