An analysis of V1065 Nova Cen 2007

Details An analysis of V1065 Nova Cen 2007 An analysis of V1065 Nova Cen 2007

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21541624v&link_type=abstract

American Astronomical Society, AAS Meeting #215, #416.24; Bulletin of the American Astronomical Society, Vol. 42, p.270

Astronomy and Astrophysics

Astronomy

Scientific paper

We present an ongoing analysis of the slow nova, v1065 Cen.  It was discovered on Jan 21, 2007, reaching a maximum magnitude of V = 8.5. The t2 time for the nova was 18 days.  We find for the ejecta a maximum expansion velocity of 4250 km/s.  Using Cloudy photoionization software to determine the physical characteristics of the ejecta, we fit multiple epochs of emission line spectra in the optical and IR, with data drawn from Spitzer and SMARTS.  Through our conclusions and their statistical significance, we present the case for an underlying ONe white dwarf.

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