Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.210..197v&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 210, Sept. 1, 1984, p. 197-221.
Astronomy and Astrophysics
Astronomy
36
Dwarf Novae, Stellar Flares, Ultraviolet Astronomy, Bursts, Continuous Spectra, Interstellar Extinction, Light Curve, Stellar Spectra
Scientific paper
The authors present spectroscopic and photometric observations in the optical and ultraviolet wavelength regions made during outbursts of the three dwarf novae UZ Serpentis, RX Andromedae and AH Herculis. The observations do not cover the rapid initial rise to outburst, but rather the peak and the subsequent decline. The overall changes of the continuum distributions are different in the three objects, and for UZ Ser the authors present evidence that the distribution repeats from outburst to outburst, although the line strengths do not. The decline from outburst is characterized by a drop in flux at all wavelengths, the drop being faster at shorter wavelengths. The spectrum of RX And observed at the decline is similar to that taken by Klare et al. at the same optical brightness but during a prolonged standstill.
Argyle Robert W.
Echevarria J. J.
Jones H. P. D.
La Dous Constanze
Pringle James E.
No associations
LandOfFree
Dwarf novae in outburst - Simultaneous ultraviolet and optical observations of UZ Serpentis, RX Andromedae and AH Herculis 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 Dwarf novae in outburst - Simultaneous ultraviolet and optical observations of UZ Serpentis, RX Andromedae and AH Herculis, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dwarf novae in outburst - Simultaneous ultraviolet and optical observations of UZ Serpentis, RX Andromedae and AH Herculis will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1396572