A CO J = 2-1 survey of type I post-main-sequence nebulae

Bibcode
1989A&A...218..257P
Phillips, J. P.; Mampaso, A.
Bibliographical reference

Astronomy and Astrophysics (ISSN 0004-6361), vol. 218, no. 1-2, July 1989, p. 257-263. Research supported by CAICYT and SERC.

Advertised on:
7
1989
Number of authors
2
IAC number of authors
1
Citations
6
Refereed citations
6
Description
Nine type I post-main-sequence nebulae were observed in CO J = 2-1 using the NRAO 12-m antenna at Kitt Peak. It is found that, at the most, 20 percent of type I sources have antenna temperatures of greater than 0.2 K. The results suggest secondary kinematic splitting of the primary emission shell, and confirm the presence of high velocity outflows distinguished by an anomalous spatiokinematic morphology.
Type
Refereed
Nebulae
Brightness temperature

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