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Issue A&A
Volume 410, Number 2, November I 2003
Page(s) 663 - 669
Section Stellar atmospheres
DOI http://dx.doi.org/10.1051/0004-6361:20031278



A&A 410, 663-669 (2003)
DOI: 10.1051/0004-6361:20031278

Binaries discovered by the SPY project

III. HE 2209-1444: A massive, short period double degenerate
C. A. Karl1, R. Napiwotzki1, G. Nelemans2, N. Christlieb3, D. Koester4, U. Heber1 and D. Reimers3

1  Dr.-Remeis-Sternwarte, Astronomisches Institut der Universität Erlangen-Nürnberg, Sternwartstr. 7, 96049 Bamberg, Germany
2  Institute of Astronomy, Madingley Road, CB3 0HA, Cambridge, UK
3  Hamburger Sternwarte, Universität Hamburg, Gojenbergsweg 112, 21029 Hamburg, Germany
4  Institut für Theoretische Physik und Astrophysik, Universität Kiel, 24098 Kiel, Germany

(Received 20 March 2003 / Accepted 12 August 2003 )

Abstract
In the course of our search for double degenerate (DD) binaries as potential progenitors of type Ia supernovae with the UVES spectrograph at the ESO VLT (ESO SN Ia Progenitor surveY - SPY) we discovered HE 2209-1444 to be a double-lined system consisting of two DA white dwarfs. From the analysis of the radial velocity curve we determined the period of the system to be $P = 6^{\rm h}38^{\rm m}47^{\rm s}$. The semi-amplitudes for both individual components are 109 km s -1 each. A model atmosphere analysis enabled us to derive individual temperatures for both components (8490 K and 7140 K, resp.) and masses of $0.58~M_\odot$ for each component. The total mass of the system is $1.15\pm 0.07~M_\odot$. The system will lose angular momentum due to gravitational wave radiation and therefore will merge within 5 Gyrs - less than a Hubble time. HE 2209-1444 is the second massive, short period double degenerate detected by SPY. Its total mass is about 20% below the Chandrasekhar mass limit and therefore it does not qualify as a potentional SN Ia progenitor. However, together with our previous detections it supports the view that Chandrasekhar mass systems do exist.


Key words: stars: binaries: close -- stars: supernovae: general -- stars: white dwarfs

Offprint request: C. A. Karl, karl@sternwarte.uni-erlangen.de

SIMBAD Objects



© ESO 2003


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