Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3193
Title: Post-Maximum Optical and Infrared Observations of Nova V1425 Aquilae 1995
Authors: Kamath, U. S
Anupama, G. C
Ashok, N. M
Chandrasekhar, T
Keywords: NOVAE
Issue Date: Dec-1997
Publisher: American Astronomical Society
Citation: Astronomical Journal, Vol. 114, No. 6, pp. 2671 - 2678
Abstract: We present the post-maximum optical spectroscopy and infrared photometry of Nova V1425 Aquilae 1995. The data indicate that the nova belongs to the Fe ii class and that it formed an optically thin dust shell at a very early phase compared to other dust forming novae of the same class. The total dust mass is very low with a dust-to-gas ratio of ±10/Sub -3. The optical spectrum and its evolution are similar to other Fe II novae. An extinction of EB - V 0.76 is derived from the He I line ratios and a distance of 2.7 kpc is estimated from the magnitude-decay time relations.
URI: http://hdl.handle.net/2248/3193
ISSN: 0004-6256
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Appears in Collections:IIAP Publications

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