SIMBAD references

2008MNRAS.387..344M - Mon. Not. R. Astron. Soc., 387, 344-348 (2008/June-2)

Optical evolution of Nova Ophiuchi 2007 = V2615 Oph.

MUNARI U., HENDEN A., VALENTINI M., SIVIERO A., DALLAPORTA S., OCHNER P. and TOMASONI S.

Abstract (from CDS):

The moderately fast Nova Oph 2007 reached maximum brightness on 2007 March 28 at V = 8.52, B - V = +1.12, V - RC = +0.76, V - IC= +1.59 and RC- IC= +0.83, after fast initial rise and a pre-maximum halt lasting a week. Decline times were tV2= 26.5, tB2= 30, tV3 = 48.5 and tB3= 56.5 d. The distance to the nova is d = 3.7±0.2 kpc, the height above the Galactic plane is z = 215 pc, the reddening is E(B - V) = 0.90 and the absolute magnitude at maximum is MmaxV= -7.2 and MmaxB= -7.0. The spectrum four days before maximum resembled a F6 supergiant, in an agreement with broad-band colours. It later developed into that of a standard `FeII'-class nova. Nine days past maximum, the expansion velocity estimated from the width of Hα emission component was ∼730 km/s, and the displacement from it of the principal and diffuse-enhanced absorption systems was ∼650 and 1380 km/s, respectively. Dust probably formed and disappeared during the period from 82 to 100 d past maximum, causing (at peak dust concentration) an extinction of ΔB = 1.8 mag and an extra ΔE(B - V) = 0.44 reddening.

Abstract Copyright: © 2008 The Authors. Journal compilation © 2008 RAS

Journal keyword(s): novae, cataclysmic variables

VizieR on-line data: <Available at CDS (J/MNRAS/387/344): table1.dat>

Simbad objects: 3

goto Full paper

goto View the references in ADS

To bookmark this query, right click on this link: simbad:2008MNRAS.387..344M and select 'bookmark this link' or equivalent in the popup menu