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A new hot subdwarf

Document type: Comunicacion

Abstract

HD 49798 was found to be a hot subdwarf. It is, at the present time the brightest member of this group and also the only one known spectroscopic binary. The complete paper will appear in the "Publications of the Astronomical Society of the Pacific".

General information

Issue date: 1963
Document language: English
Journal: Boletín de la Asociación Argentina de Astronomía; no. 6
Event: VI Reunión Científica de la Asociación Argentina de Astronomía (Horco Molle, Tucumán, 22 al 25 de mayo de 1963)
Origin: Asociación Argentina de Astronomía
Pages: 32-32
xmlui.dri2xhtml.METS-1.0.item-dc-subject: estrella subenana
Subjects: Ciencias Astronómicas

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Created: 25 de marzo de 2020
Available since: 25 de marzo de 2020
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