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Visible and/or near infrared spectral variations of v1016 Cygni, HM sagittae and MWC 349
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 g...
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Published in: | Astrophysics and space science 1982-04, Vol.83 (1-2), p.423-435 |
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Main Authors: | , , |
Format: | Article |
Language: | English |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | 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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ISSN: | 0004-640X 1572-946X |
DOI: | 10.1007/BF00648571 |