Visible and/or near infrared spectral variations of V1016 Cygni, HM Sagittae and MWC 349

Details Visible and/or near infrared spectral variations of V1016 Cygni, HM Sagittae and MWC 349 Visible and/or near infrared spectral variations of V1016 Cygni, HM Sagittae and MWC 349

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..83..423a&link_type=abstract

Astrophysics and Space Science, vol. 83, no. 1-2, Apr. 1982, p. 423-435. Research supported by the Consiglio Nazionale delle Ri

Astronomy and Astrophysics

Astrophysics

19

Emission Spectra, Infrared Stars, Peculiar Stars, Stellar Evolution, Stellar Spectra, Variable Stars, Hot Stars, Light (Visible Radiation), Line Spectra, Near Infrared Radiation, Spectrum Analysis

Scientific paper

The recent spectral evolution of the three peculiar emission-line objects with IR excess V1016 Cyg, HM Sge, and MWC 349 is described using data obtained at the Asiago (blue and red spectral regions) and Haute Provence (near infrared) observatories. In the near infrared spectral region, details are given concerning the data briefly described by Andrillat and Swings (1980).

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