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Sirius Matters [electronic resource] / by Noah Brosch.

Por: Tipo de material: TextoTextoSeries Astrophysics and Space Science Library ; 354 | Astrophysics and Space Science Library ; 354Editor: Dordrecht : Springer Netherlands, 2008Descripción: XVII, 216 p. online resourceTipo de contenido:
  • text
Tipo de medio:
  • computer
Tipo de soporte:
  • online resource
ISBN:
  • 9781402083198
Trabajos contenidos:
  • SpringerLink (Online service)
Tema(s): Formatos físicos adicionales: Sin títuloClasificación CDD:
  • 520 23
Clasificación LoC:
  • QB4
Recursos en línea:
Contenidos:
Springer eBooksResumen: Since very early times Sirius was a point of attraction in the night sky. It served to synchronize calendars in antiquity and was the subject of many myths and legends, including some modern ones. It was perceived as a red star for more than 400 years, but such reports were relegated to the Mediterranean region. Astronomically, Sirius is a very bright star. This, and its present close distance to us, argues in favor of it being the target of detailed studies of stellar structure and evolution. Its binary nature, with a companion that is one of the more massive white dwarfs, is an additional reason for such studies. This book collects the published information on Sirius in an attempt to derive a coherent picture of how this system came to look as it does.
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Historical perspective -- Mysteries of the Sirius system -- Approaching modern times -- Modern optical measurements -- Modern non-optical observations -- The neighborhood of Sirius -- The perspective of stellar structure -- The perspective of stellar evolution -- Sirius revealed a synthesis of the information.

Since very early times Sirius was a point of attraction in the night sky. It served to synchronize calendars in antiquity and was the subject of many myths and legends, including some modern ones. It was perceived as a red star for more than 400 years, but such reports were relegated to the Mediterranean region. Astronomically, Sirius is a very bright star. This, and its present close distance to us, argues in favor of it being the target of detailed studies of stellar structure and evolution. Its binary nature, with a companion that is one of the more massive white dwarfs, is an additional reason for such studies. This book collects the published information on Sirius in an attempt to derive a coherent picture of how this system came to look as it does.

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