| Titre : |
Studies on transient X-ray sources with the Ariel 5 all-sky monitor |
| Type de document : |
texte imprimé |
| Auteurs : |
Louis Joseph Kaluzienski, Auteur ; University of Maryland, Organisme de soutenance |
| Editeur : |
Greenbelt , Md. : NASA Goddard Space Flight Center |
| Année de publication : |
1977 |
| Collection : |
X (Goddard Space Flight Center) num. 661-77-107 |
| Importance : |
1 vol. (XXVII, 220 p.) |
| Présentation : |
ill., diagrs., graphs |
| Format : |
27 cm |
| ISBN/ISSN/EAN : |
PPN 193177595 |
| Note générale : |
Dissertation submitted to the Faculty of the Graduate School of the University of Maryland : 1977. - "Supported by NASA Grant NGR 21-002-316." Vita. Issued as : NASA-TM-X-71321. |
| Langues : |
Anglais (eng) |
| Tags : |
Astronomie des rayons X -- Thèses et écrits académiques Ariel (satellite artificiel) -- Thèses et écrits académiques X-ray astronomy -- Thesis Ariel (artificial satellite) -- Thesis |
| Index. décimale : |
522.686 3 Astronomie des rayons X |
| Résumé : |
The All-Sky Monitor, an imaging X-ray detector launched aboard the Ariel 5 satellite, was used to obtain detailed light curves of three new sources. Additional data essential to the determination of the characteristic luminosities, rates of occurrence (and possible recurrence), and spatial distribution of these objects was also obtained. The observations are consistent with a roughly uniform galactic disk population consisting of at least two source sub-classes, with the second group (Type 2) at least an order of magnitude less luminous and correspondingly more frequent than the first (Type 1). While both subtypes are probably unrelated to the classical optical novae (or supernovae), they are most readily interpreted within the standard mass exchange X-ray binary model, with outbursts triggered by Roche-lobe overflow (Type 1) or enhancements in the stellar wind density of the companion (Type 2), respectively. |
Studies on transient X-ray sources with the Ariel 5 all-sky monitor [texte imprimé] / Louis Joseph Kaluzienski, Auteur ; University of Maryland, Organisme de soutenance . - Greenbelt , Md. : NASA Goddard Space Flight Center, 1977 . - 1 vol. (XXVII, 220 p.) : ill., diagrs., graphs ; 27 cm. - ( X (Goddard Space Flight Center); 661-77-107) . ISSN : PPN 193177595 Dissertation submitted to the Faculty of the Graduate School of the University of Maryland : 1977. - "Supported by NASA Grant NGR 21-002-316." Vita. Issued as : NASA-TM-X-71321. Langues : Anglais ( eng)
| Tags : |
Astronomie des rayons X -- Thèses et écrits académiques Ariel (satellite artificiel) -- Thèses et écrits académiques X-ray astronomy -- Thesis Ariel (artificial satellite) -- Thesis |
| Index. décimale : |
522.686 3 Astronomie des rayons X |
| Résumé : |
The All-Sky Monitor, an imaging X-ray detector launched aboard the Ariel 5 satellite, was used to obtain detailed light curves of three new sources. Additional data essential to the determination of the characteristic luminosities, rates of occurrence (and possible recurrence), and spatial distribution of these objects was also obtained. The observations are consistent with a roughly uniform galactic disk population consisting of at least two source sub-classes, with the second group (Type 2) at least an order of magnitude less luminous and correspondingly more frequent than the first (Type 1). While both subtypes are probably unrelated to the classical optical novae (or supernovae), they are most readily interpreted within the standard mass exchange X-ray binary model, with outbursts triggered by Roche-lobe overflow (Type 1) or enhancements in the stellar wind density of the companion (Type 2), respectively. |
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trié(s) par (Pertinence décroissant(e), Titre croissant(e)) Affiner la rechercheContributions to the 1969 Budapest conference on Cosmic Rays / Goddard Space Flight Center. High-energy astrophysics branch (1969)
