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OPTISCHE SPECTROSKOPIE VON KLASSISCHEN STERNEN IN DER GALAXIE: Untersuchung stellarer gasförmiger Scheiben

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Last 91 days · 91 data points

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£77.00 £73.92 £74.59 £75.26 £75.94 £76.61 £77.28 20 July 2026 11 August 2026 03 September 2026 25 September 2026 18 October 2026
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1 day · current 90 days 0 23 45 68 90 £74 £77 Days at Price

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Most common price: £77 (90 days, 98.9%)

Price range: £74 - £77

Price levels: 2 different prices over 91 days

Description

Die spektroskopische Untersuchung von klassischen Be-Sternen (Be) ist wichtig, um die Physik ihrer Scheiben besser zu verstehen. Kürzlich erstellten Banerjee et al. (2021) einen Atlas aller wichtigen Emissionslinien, die in einer großen Stichprobe von über 100 Be-Sternen im Feld gefunden wurden, unter Verwendung des 2-m-Himalaya-Chandra-Teleskops des Indian Institute of Astrophysics (IIA) in Ladakh, Indien. Diese Studie enthüllte mehrere wichtige Aspekte der Scheiben von Be-Sternen, wie z. B. die Bedeutung der Berücksichtigung des Extinktionsparameters (AV) für die Untersuchung der Eigenschaften von Be-Sternen, die Tatsache, dass ihre Scheiben im Allgemeinen optisch dick sind, die wahrscheinliche Existenz von nicht-isothermen Scheiben in einigen dieser Sterne, die für die Produktion von Ca II-Triplett-Emissionslinien verantwortlich sein könnten, usw. In einer anderen Studie (Banerjee et al. 2022) konzentrierten wir uns auf das Verständnis der vorübergehenden Natur von Be-Sternen durch die kontinuierliche Beobachtung ihrer Hα-Linienprofile über fünf aufeinanderfolgende Jahre mit dem 1-Meter-Teleskop am Vainu Bappu Observatorium in Kavalur, Indien, das vom IIA betrieben wird. Unsere Arbeit eröffnet somit einen breiten Spielraum für die Durchführung weiterer spezieller Studien von Be-Sternen anhand größerer Stichproben, um ihre Scheibeneigenschaften besser zu verstehen.

Product Specifications

Format
paperback
Domain
Amazon UK
Release Date
15 June 2024
Listed Since
16 June 2024

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No barcode data available

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