X-ray observations of Vela-X

Autor:	A. Smith, H.U. Zimmermann
Rok vydání:	1985
Předmět:	Physics Atmospheric Science Nebula X-ray Aerospace Engineering Astronomy Astronomy and Astrophysics Astrophysics Vela Astronomical spectroscopy Geophysics Pulsar Space and Planetary Science General Earth and Planetary Sciences
Zdroj:	Advances in Space Research. 5:53-56
ISSN:	0273-1177
DOI:	10.1016/0273-1177(85)90449-1
Popis:	Exosat ME observations of the Vela-X region are presented. It is found that the 2–10 keV emission is divided into two components. One is associated with the rulsar but is probably extended by 10–20 arc minutes, the other is associated with the Vela-X radio nebula and is probably more extended ( ⪸ 1 degree ). The Vela-X component is softer than the pulsar component. No pulsed emission is observed.
Databáze:	OpenAIRE
Externí odkaz:	https://explore.openaire.eu/search/publication?articleId=doi_________::d90455c1bcc7f4ff17585ec165b42672 https://doi.org/10.1016/0273-1177(85)90449-1 Zobrazit plný text záznamu