High-resolution spectra of the luminous young stellar object V645 Cygni

Details High-resolution spectra of the luminous young stellar object V645 Cygni High-resolution spectra of the luminous young stellar object V645 Cygni

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...339.1078h&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 339, April 15, 1989, p. 1078-1088. Research supported by NSF.

Other

36

Pre-Main Sequence Stars, Stellar Envelopes, Stellar Mass Ejection, Stellar Spectra, Infrared Spectra, K Lines, Metallicity, Oxygen, Spectral Line Width

Scientific paper

The paper presents 6310-11,000 A spectra at 22, 75,and 90 km/s
resolution of the two brightest knots (N0 and N1) near the luminous
young stellar object V645 Cygni. The measured line profiles suggest a
circumstellar disk plus bipolar wind model like those proposed for other
premain-sequence stars.

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