Hostname: page-component-76fb5796d-qxdb6 Total loading time: 0 Render date: 2024-04-29T15:25:46.614Z Has data issue: false hasContentIssue false
  • English
  • Français

Infrared Spectroscopy of Nova V705 Cas

Published online by Cambridge University Press:  12 April 2016

A. Evans ,
T.R. Geballe ,
J.M.C. Rawlings  and
A.D. Scott
A. Evans
Affiliation:
Department of Physics, Keele University, UK
T.R. Geballe
Affiliation:
Joint Astronomy Centre, Hilo, Hawaii, USA
J.M.C. Rawlings
Affiliation:
Department of Physics & Astronomy, University College, London, UK
A.D. Scott
Affiliation:
Department of Physics, Keele University, UK

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Nova V705 Cas was discovered on 1993 December 7, several days before maximum light. The light curve indicates that t2 ≃ 40 d (see e.g. [4]), characteristic of dust-forming novae. The light curve went into decline on day 58, indicating the formation of an optically thick dust shell. IR spectra have been obtained regularly since outburst using the cooled grating spectrometer CGS4 on the United Kingdom InfraRed Telescope (UKIRT). We present here the results of ongoing IR spectroscopic monitoring of this nova.

Type
Novae & Symbiotic Stars
Information
International Astronomical Union Colloquium , Volume 158: Cataclysmic Variables and Related Objects , 1996 , pp. 325 - 326
Copyright
Copyright © Kluwer 1996

References

1. Evans, A., Geballe, T.R., Rawlings, J.M.C., Scott, A.D., 1996, MNRAS, in pressGoogle Scholar
2. Evans, A., Rawlings, J.M.C., 1994, MNRAS, 269, 427 Google Scholar
3. Greenhouse, M.A., Grasdalen, G.L., Woodward, C.E. et al., 1990, Ap. J., 352, 307 Google Scholar
4. Petrík, K., Hric, L., Urban, Z., et al., 1996, these proceedings, p323CrossRefGoogle Scholar
5. Rawlings, J.M.C., 1988, MNRAS, 232, 507 CrossRefGoogle Scholar
6. Rawlings, J.M.C., Williams, D.A., 1989, MNRAS, 240, 729 Google Scholar