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Beschreibung
Once you have looked at the night sky on a moonless night it is not hard to realise why so much of our science and religion has its roots in the stars. Yet it took until 1850 to realise that fainter stars were not necessarily further away, nor the brighter ones closer. In fact within the magnitude range observable to the naked eye it is probable that the brighter star is in fact further away. Even… today the measurement of stellar distances is relatively difficult and is gener ally only done using dedicated telescopes. In the early years of the 20th century Hertzsprung and Russell developed a powerful classification diagram which al lows stars to be distinguished using a plot of their colour versus magnitude. The construction of this diagram involved the use of spectroscopy which has become the cornerstone of modern astronomy. As telescopes become more powerful, de tectors more sensitive and more physics is added to astrophysics, astronomical spectroscopy becomes a more powerful tool. The concern of this book is the spectral classification of stars. With a single spectrum of a star it is possible to uniquely classify an object and find its place on the Hertzsprung-Russell diagram. This spectrum is thus equivalent to having the colour and the magnitude of the object which can in turn be related to mass and other quantities. 106,99 €
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Technische Daten
Erscheinungsdatum
07.11.2012
Sprache
Englisch
EAN
9783642626821
Herausgeber
Springer Berlin
Sonderedition
Nein
Seitenanzahl
197
Auflage
1
Einbandart
Broschiert
Buch Untertitel
New Spectral Types L and T
Schlagwörter
Brown Dwarf, Mass Function, Spectral Classification, Ultracool Dwarf, stellar
Thema-Inhalt
PGG - Astronomische Beobachtung: Observatorien, Ausrüstungen und Methoden
PHVB - Astrophysik
Höhe
235 mm
Breite
15.5 cm
Transparenz & Sicherheit
Hersteller: Springer, Europaplatz 3, Heidelberg, Deutschland, 69115, ProductSafety@springernature.com, Springer Nature Customer Service Center GmbH
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