Near Infrared Observations of the novae V2491 Cygni and V597 Puppis

Abstract

We present results obtained from near-infrared JHK spectroscopic observations of novae V2491 Cyg and V597 Pup in the early declining phases of their 2007 and 2008 outbursts respectively. In both objects, the spectra displayed emission lines of HI, OI, HeI and NI. In V597 Pup, the HeI lines were found to strengthen rapidly with time. Based on the observed spectral characteristics, both objects are classified as He/N novae. We have investigated the possibility of V2491 Cyg being a recurrent nova as has been suggested. By studying the temporal evolution of the line widths in V2491 Cyg it appears unlikely that the binary companion is a giant star with heavy wind as in recurrent novae of the RS Oph type. Significant deviations from that of recombination case B conditions are observed in the strengths of the HI lines. This indicates that the HI lines, in both novae, are optically thick during the span of our observations. The slope of the continuum spectra in both cases was found to have a λ^-(3-3.5) dependence which deviates from a Rayleigh-Jeans spectral distribution. Both novae were detected in the post-outburst super-soft X-ray phase; V2491 Cyg being very bright in X-rays has been the target of several observations. We discuss and correlate our infrared observations with the observed X-ray properties of these novae.

9 pages, 7 figures, Accepted for publication in MNRAS

References in corpus (6)

• A near-infrared shock wave in the 2006 outburst of recurrent nova RS Ophiuchi
• Near-Infrared Studies of V1280 Sco (Nova Scorpii 2007)
• VLTI monitoring of the dust formation event of the Nova V1280 Sco
• Prediction of Supersoft X-ray Phase during the 2006 Outburst of RS Ophiuchi
• The unusual Nova Cygni 2006 (V2362 Cyg)
• Near-Infrared and Optical Studies of the fast nova V4643 Sgr (Nova Sagittarii 2001)

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• The $UBV$ Color Evolution of Classical Novae. IV. Time-Stretched $(U-B{)}_0$-$(M_B-2.5\log f_{\mathrm{s}})$ and $(V-I{)}_0$-$(M_I-2.5\log f_{\mathrm{s}})$ Color-Magnitude Diagrams of Novae in Outburst
• Infrared spectroscopy of the 2019 eruption of the recurrent nova V3890 Sgr: separation into equatorial and polar winds revealed