Hostname: page-component-77c89778f8-cnmwb Total loading time: 0 Render date: 2024-07-18T00:58:44.688Z Has data issue: false hasContentIssue false
  • English
  • Français

Interferometric images of 13CO emission toward HL Tau

Published online by Cambridge University Press:  04 August 2017

Steven Beckwith  and
Anneila Sargent
Steven Beckwith
Affiliation:
MPI fur Astronomie and Owens Valley Radio Observatory
Anneila Sargent
Affiliation:
MPI fur Astronomie and Owens Valley Radio Observatory

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Millimeter wave interferometric images of HL Tau show a clear disk morphology with a nearly keplerian velocity curve. A few a few tenths of a solar mass are in orbit around the star.

Type
Bipolar Flows, Jets and Protostars
Information
Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 81 - 83
Copyright
Copyright © Reidel 1987 

References

Beckwith, S., Sargent, A.I., Scoville, N.Z., Masson, C.R., Zuckerman, B., and Phillips, T.G. 1986, Ap. J., in press.Google Scholar
Beckwith, S., Zuckerman, B., Skrutskie, M.F., and Dyck, H.M. 1984, Ap. J., 287, 793.CrossRefGoogle Scholar
Cohen, M. 1983, Ap. J. (Letters), 270, L69.CrossRefGoogle Scholar
Hildebrand, R.H. 1983, Quart. Journ. R.A.S., 24, 267.Google Scholar
Hodapp, K.W. 1984, Astron. Ap., 141, 255.Google Scholar
Mundt, R. and Fried, J.W. 1983, Ap. J. (Letters), 274, L83.CrossRefGoogle Scholar
Sargent, A.I. and Beckwith, S. 1986, in preparation.Google Scholar
Snell, R., Loren, R., and Plambeck, R. 1980, Ap. J. (Letters), 239, L17.CrossRefGoogle Scholar