A spectrum of the symbiotic Nova RT Serpentis

Details A spectrum of the symbiotic Nova RT Serpentis A spectrum of the symbiotic Nova RT Serpentis

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pasp...97..151m&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 97, Feb. 1985, p. 151, 152.

Astronomy and Astrophysics

Astronomy

2

Novae, Stellar Spectra, Symbiotic Stars, Emission Spectra, H Alpha Line, Helium, Radial Velocity

Scientific paper

The spectrum of RT Ser (Nova Serpentis 1909) was observed in 1979 in the range 6300 Å to 6750 Å, at a resolution of 0.6 Å. In addition to the dominant Hα line, weak emission lines of [O I] λ6363 and He I λ6678 were detected. These lines have radial velocities of 64, 82, and 77 km s-1, respectively. Emitting regions with different physical conditions around RT Ser appear to have different radial velocities.

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