Condensations in the planetary nebula NGC 7293 - an origin in circumstellar SiO maser spots?

Details Condensations in the planetary nebula NGC 7293 - an origin in circumstellar SiO maser spots? Condensations in the planetary nebula NGC 7293 - an origin in circumstellar SiO maser spots?

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.241..625d&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 241, Dec. 15, 1989, p. 625-630.

Astronomy and Astrophysics

Astronomy

74

Interstellar Masers, Planetary Nebulae, Red Giant Stars, Silicon Oxides, Starspots, Condensation, Stellar Mass Ejection, Stellar Winds

Scientific paper

NGC 7293 is a planetary nebula containing numerous clumps of gas having linear sizes of about 0.001 pc. It is argued that these clumps are cold (T about 10 K), dense (n about 10 to the 6th/cu cm), and molecular. The survival of clumps during the different stellar mass-loss phases associated with planetary nebula nucleus evolution is considered; it is speculated that the clumps were associated with circumstellar SiO maser spots.

Affiliated with

Also associated with

No associations

Rating

Condensations in the planetary nebula NGC 7293 - an origin in circumstellar SiO maser spots? does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Condensations in the planetary nebula NGC 7293 - an origin in circumstellar SiO maser spots?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Condensations in the planetary nebula NGC 7293 - an origin in circumstellar SiO maser spots? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1575422