OPTICAL MORPHOLOGY, INCLINATION, AND EXPANSION VELOCITY OF THE EJECTED SHELL OF NOVA MONOCEROTIS 2012

Journal article

Authors/Editors

Ribeiro, Valério

Research Areas

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Publication Details

Author list: Ribeiro VARM, Munari U, Valisa P

Publisher: American Astronomical Society

Place: BRISTOL

Publication year: 2013

Journal: The Astrophysical Journal (0004-637X)

Journal acronym: ASTROPHYS J

Volume number: 768

Issue number: 1

Number of pages: 7

ISSN: 0004-637X

eISSN: 1538-4357

Languages: English-Great Britain (EN-GB)

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Abstract

The morphology of the ejected shell of the He/N Nova Monocerotis 2012 outburst was studied in detail. Synthetic line profile spectra were compared to the [OIII] 4959, 5007 angstrom emission line profiles in order to find the best-fit morphology, an inclination angle, and a maximum expansion velocity of the ejected shell. The simplest morphology was found to be that of a bipolar structure with an inclination angle of 82 degrees +/- 6 degrees and a maximum expansion velocity of 2400(-200)(+300) km s(-1) (at day 130 after outburst). Such a high degree of shaping is unexpected for a system with a main-sequence star (as suspected from the systems colors). The degree of shaping may be disentangled with resolved optical imaging. Furthermore, these results may be confirmed with radio imaging which is expected to follow the same gross features of the outburst as the optical band and the high inclination implied here can be corroborated with a 7.1 hr period which has been suggested to arise from partial eclipses of extended emission by an accretion disk rim.

Keywords

novae, cataclysmic variables, stars: individual (Nova Mon 2012)

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