Nova Aquilae 1982

Details Nova Aquilae 1982 Nova Aquilae 1982

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987mnras.228..329s&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 228, Sept. 15, 1987, p. 329-376.

Astronomy and Astrophysics

Astronomy

73

Light Curve, Novae, Radio Spectra, Stellar Spectrophotometry, Ultraviolet Spectra, Interstellar Extinction, Iue, Line Shape, Radiant Flux Density, Spaceborne Astronomy

Scientific paper

Observations of Nova Aquilae obtained from the IUE, the Anglo-Australian Telescope, and the Westerbork Synthesis Radio Telescope are discussed. Light curves for B, V, and continuum fluxes at 2800 and 1300 A are presented. Velocities obtained from line profiles indicate the presence of three main gaseous components: a high velocity gas (HVG) component found only in absorption lines on D = 29 and 35, and a medium-velocity gas (MVG) and low-velocity gas component found in emission lines and, for the MVG, in the Na I D-line absorption. A model for thermal emission from the HVG is discussed. It is suggested that ionization in the MVG was maintained by photoionization. Properties of the dust grains are studied using data from absorption in the optical and UV and from emission in the IR.

Affiliated with

Also associated with

No associations

Rating

Nova Aquilae 1982 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Nova Aquilae 1982, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Nova Aquilae 1982 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1676541