Radio and infrared structures of type I post-main sequence nebulae

Bibcode
1988A&A...190..237P
Phillips, J. P.; Mampaso, A.
Bibliographical reference

Astronomy and Astrophysics (ISSN 0004-6361), vol. 190, no. 1-2, Jan. 1988, p. 237-258. Research supported by the Science Research Council of England and CAICYT.

Advertised on:
1
1988
Number of authors
2
IAC number of authors
1
Citations
35
Refereed citations
34
Description
High-resolution VLA radio mapping at 1.46, 4.84, and 15.0 GHz is presented together with NIR J,H,K,L, and M mapping and photometry of a broad range of type I postmain-sequence nebulae. Many of these sources have extremely compact infrared and radio cores ranging from 0.1 to 0.01 pc in size; in some cases they contain up to 96 percent of the total radio flux. A detailed investigation of the IRAS photometry for type I nebulae was undertaken; a typical interior grain temperature is estimated to be 200 K while outer shell temperatures are estimated to be less than 50 K.
Type
Refereed
Nebulae

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