MWC 349, an optical, radio, and infrared source
Journal Article
·
· Astrophys. J., Lett., v. 184, no. 1, pp. L23-L27
Optical multichannel photometry is combined with radio infrared data on MWC 349. The optical continuum and line emission varied in 24 hours. A very reddened, probably hot star coexists with a small H ii region of high electron density, a dust cloud (radiating above 1 mu ), and (probably) an inhomogeneous themal radio source. A tentative model is described. (auth)
- Research Organization:
- Hale Observatories, California Institute of Technology, Carnegie Institution of Washington
- Sponsoring Organization:
- USDOE
- NSA Number:
- NSA-29-013482
- OSTI ID:
- 4380322
- Journal Information:
- Astrophys. J., Lett., v. 184, no. 1, pp. L23-L27, Journal Name: Astrophys. J., Lett., v. 184, no. 1, pp. L23-L27; ISSN AJLEA
- Country of Publication:
- United States
- Language:
- English
Similar Records
MWC 349 - a bipolar nebula with a very hot central star
CO AND H{sup +}{sub 3} TOWARD MWC 1080, MWC 349, AND LkH{alpha} 101
VLA observations of MWC 349 at 15 and 23 GHz
Journal Article
·
Tue Oct 01 00:00:00 EDT 1985
· Astrophys. J.; (United States)
·
OSTI ID:5556524
CO AND H{sup +}{sub 3} TOWARD MWC 1080, MWC 349, AND LkH{alpha} 101
Journal Article
·
Tue Jun 01 00:00:00 EDT 2010
· Astrophysical Journal
·
OSTI ID:21450938
VLA observations of MWC 349 at 15 and 23 GHz
Journal Article
·
Fri Jul 01 00:00:00 EDT 1983
· Astron. J.; (United States)
·
OSTI ID:5961339