The Early Type Stars

A. B. Underhill

ISBN 10: 9027701415 / ISBN 13: 9789027701411

Edité par Springer Netherlands, Springer Netherlands Jul 1966, 1966

A propos de cet article

This item is printed on demand - Print on Demand Titel. Neuware -At this time when astronomers are being surprised by the discovery of objects which emit a fabulously large amount of energy, that is the quasi-stellar radio sources and the quasi-stellar galaxies, and when by the means of space vehicles X rays, gamma rays and cosmic rays are being observed to come from the depths of interstellar space, one may ask why write a book about stars. Stars seem to be almost incidental when one looks at the universe in terms of exceedingly great energies. Nevertheless, stars exist. They are accessible to study and they have not yet revealed all their secrets. This is enough to arouse interest and to cause one to try to find answers to the questions which arise. The early type stars are particularly interesting because they are spendthrift stars pouring out their energy at a great rate. But their brilliance is also their undoing. They must evolve rather quickly, on an astrophysical scale. Thus by studying these stars we are studying a population in change. The implications from the local and from the cosmological viewpoint are important if one wishes to understand the details of stellar evolution and of galactic structure. Perhaps one of the simplest reasons for writing a book about the early type stars is to see if some of the conundrums pre sented by the spectra of these stars can be unravelled when all the available infor mation is brought together.Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg 300 pp. Englisch.

N° de réf. du vendeur 9789027701411

Détails bibliographiques

• Titre: The Early Type Stars
• Éditeur: Springer Netherlands, Springer Netherlands Jul 1966
• Date de parution: 1966
• Langue: anglais
• ISBN à 10 chiffres: 9027701415
• ISBN à 13 chiffres: 9789027701411
• Reliure: Buch
• État de l'article: Neu
• Dimensions: 241 L x 160 H x 21 P (en millimètres) 241 millimètres de largeur par 160 millimètres de hauteur par 21 millimètres de profondeur
• Poids: 617 grammes

A propos de ce titre

Synopsis

At this time when astronomers are being surprised by the discovery of objects which emit a fabulously large amount of energy, that is the quasi-stellar radio sources and the quasi-stellar galaxies, and when by the means of space vehicles X rays, gamma rays and cosmic rays are being observed to come from the depths of interstellar space, one may ask why write a book about stars. Stars seem to be almost incidental when one looks at the universe in terms of exceedingly great energies. Nevertheless, stars exist. They are accessible to study and they have not yet revealed all their secrets. This is enough to arouse interest and to cause one to try to find answers to the questions which arise. The early type stars are particularly interesting because they are spendthrift stars pouring out their energy at a great rate. But their brilliance is also their undoing. They must evolve rather quickly, on an astrophysical scale. Thus by studying these stars we are studying a population in change. The implications from the local and from the cosmological viewpoint are important if one wishes to understand the details of stellar evolution and of galactic structure. Perhaps one of the simplest reasons for writing a book about the early type stars is to see if some of the conundrums pre- sented by the spectra of these stars can be unravelled when all the available infor- mation is brought together.