The equilibrium structure of a thin magnetic flux tube. III - The effects of molecular CO absorption

Details The equilibrium structure of a thin magnetic flux tube. III - The effects of molecular CO absorption The equilibrium structure of a thin magnetic flux tube. III - The effects of molecular CO absorption

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...333..925m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 333, Oct. 15, 1988, p. 925-935. Research supported by the Ministero della P

Astronomy and Astrophysics

Astrophysics

7

Carbon Monoxide, Late Stars, Magnetic Flux, Molecular Structure, Stellar Atmospheres, Atmospheric Temperature, Magnetic Stars, Surface Temperature

Scientific paper

The authors determine the structure of a stellar atmosphere and of a thin magnetic flux tube embedded in it, taking the opacity by H- and carbon monoxide into account. It is found that CO has a strong cooling effect on the external atmosphere. For effective temperatures below ≡5900K, the surface temperature of the atmosphere with H- and CO opacity is much lower than with H- alone. In the interior of the flux tube the equations can have multiple solutions. Thus hot flux tubes can exist in a cool atmosphere even in the absence of nonradiative heating.

Affiliated with

Also associated with

No associations

Rating

The equilibrium structure of a thin magnetic flux tube. III - The effects of molecular CO absorption 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 The equilibrium structure of a thin magnetic flux tube. III - The effects of molecular CO absorption, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The equilibrium structure of a thin magnetic flux tube. III - The effects of molecular CO absorption will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1598210