Optical Spectroscopy of the Unusual Emission-Line Object MWC 560

Astronomy and Astrophysics – Astronomy

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MWC 560, classified Beq in the original Mt. Wilson survey but noted as type M4ep by Sanduleak and Stephenson (Ap.J. 185, 899), underwent an outburst in 1990. Between Feb.-Apr. 1990 the star showed dramatic UV spectral variability, indicating the ejection of a thick shell (Michalitsianos et al., Ap.J. 371, 761). We have monitored the optical spectrum of MWC 560 during 1990-92 at Ritter Observatory using a fiber-coupled spectrograph and CCD, in coordination with IUE. Very significant spectral changes took place between the 90/91 and 91/92 observing seasons. Compared with 90/91, the data from a year later show: a broader and more blueshifted (-2200 km/s) absorption component of the strong Hα emission line; weaker Fe II, O I, and He I emission lines; much weaker D-line absorption. In the 8000-9000 Angstroms region, the Ca II infrared triplet lines are strong, narrow emission features, superimposed on the continuum of an M5 star; TiO bandheads appear stronger in 91/92 than a year earlier. The visible/red spectrum of MWC 560 appears to have been dominated by optically thick shell features in late-1990/early-1991. By November 1991, the shell signatures have weakened, and a variable high-velocity wind profile is evident at Hα . This research was partially supported by grants from NASA.

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