Hostname: page-component-586b7cd67f-rcrh6 Total loading time: 0 Render date: 2024-11-27T01:50:11.604Z Has data issue: false hasContentIssue false

SMA imaging of the masers in MWC349A

Published online by Cambridge University Press:  01 March 2007

Jonathan Weintroub*
Affiliation:
Harvard-Smithsonian CfA, 60 Garden Street, MS78, Cambridge, MA 02138, USA email: [email protected]
James Moran
Affiliation:
Harvard-Smithsonian CfA, 60 Garden Street, MS78, Cambridge, MA 02138, USA email: [email protected]
Ramprasad Rao
Affiliation:
ASIAA, 645 North A'ohoku Place, Hilo, Hawaii 96720
Hiroko Shinnaga
Affiliation:
Caltech Submillimeter Observatory, 111 Nowelo Street, Hilo, HI 96720
David Wilner
Affiliation:
Harvard-Smithsonian CfA, 60 Garden Street, MS78, Cambridge, MA 02138, USA email: [email protected]
Ken Young
Affiliation:
Harvard-Smithsonian CfA, 60 Garden Street, MS78, Cambridge, MA 02138, USA email: [email protected]
Rights & Permissions [Opens in a new window]

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.

In September 2004 and September 2005 we used the Submillimeter Array (SMA) to map the distribution of hydrogen recombination line (HRL) maser spots that originate in the envelope of the peculiar star MWC349A. We measured positions in the line over a 100 km/s velocity range with 1 km/s spectral resolution. Relative angular position was estimated to an accuracy of about 0.01 arcseconds. The H30α maser components can be tracked continuously in frequency between the red- and blue-shifted peaks of the spectrum. The masers appear to trace a nearly edge-on disk-like structure. The position-velocity relationship is quite remarkable, and reminiscent of that of NCG4258. However, the “wings” in the PV relation are too steep for a simple Keplerian prescription to be correct. We present our data, and suggest a simple model to account for the steep wings.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2008

References

Danchi, W. C., Tuthill, P. G., & Monnier, J. D. 2001, ApJ 562, 440Google Scholar
Planesas, P., Martín-Pintado, J., & Serabyn, E. 1992, ApJ, 386, L23CrossRefGoogle Scholar
Tafoya, D., Gómez, Y., & Rodríguez, L. F. 2004, ApJ 610, 827CrossRefGoogle Scholar
White, R. L. & Becker, P. H. 1985, ApJ, 297, 677Google Scholar