Nova 1670 Vul

M. Hajduk, Albert A. Zijlstra, A. Evans, F. Kerber, P. A. M. Van Hoof, Don L Pollacco, Stewart Eyres, S. Kimeswenger, K. Gesicki

Allbwn ymchwil: Pennod mewn Llyfr/Adroddiad/Trafodion CynhadleddCyfraniad i gynhadleddadolygiad gan gymheiriaid

Crynodeb

We present radio and optical observations of CK Vul, an object associated with a nova-like outburst observed in 1670�1672. A barely resolved point source, detected at radio wavelengths, suggests thermal emission at the presumed position of the central star, which remains undetected in the optical region. The measured proper motion of the nebula confirms that the observed object is indeed the remnant of the 1670 eruption. We also report the discovery of an extended bipolar nebula, ejected in the same time.
Iaith wreiddiolSaesneg
TeitlAstronomical Society of the Pacific Conference Series
Is-deitlWhy Galaxies Care About AGB Stars: Their Importance as Actors and Probes
GolygyddionF. Kerschbaum, C. Charbonnel, R. F. Wing
CyhoeddwrAstronomical Society of the Pacific
Tudalennau301
Cyfrol378
ISBN (Electronig)978-1-58381-319-5
ISBN (Argraffiad)978-1-58381-318-8
StatwsCyhoeddwyd - 2007
DigwyddiadAstronomical Society of the Pacific Conference 2006: Why Galaxies Care About AGB Stars: Their Importance as Actors and Probes - University Campus, Vienna, Awstria
Hyd: 7 Aug 200611 Aug 2006

Cynhadledd

CynhadleddAstronomical Society of the Pacific Conference 2006
Gwlad/TiriogaethAwstria
DinasVienna
Cyfnod7/08/0611/08/06

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