Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...165..157m&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 165, no. 1-2, Sept. 1986, p. 157-162.
Astronomy and Astrophysics
Astrophysics
54
Corotation, Early Stars, Stellar Mass Ejection, Stellar Winds, Ultraviolet Absorption, Ultraviolet Spectra, Astronomical Models, Iue, Magnetohydrodynamic Flow, Spectrum Analysis
Scientific paper
The discovery of displaced narrow components (DNCs) in an increasingly large number of stars of various spectral types suggests that an explanation of these features may contribute significantly to understanding of winds from stars of all types. The reported properties of DNCs are summarized here with a view to evaluating one particular scenario for DNC formation which involves corotating interaction regions (CIRs) in the stellar wind. The relevant features of the CIR scenario are summarized, and the extent to which DNC properties support the CIR scenario is discussed.
No associations
LandOfFree
Displaced narrow absorption components in the spectra of mass-losing OB stars - Indications of corotating interaction regions? 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 Displaced narrow absorption components in the spectra of mass-losing OB stars - Indications of corotating interaction regions?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Displaced narrow absorption components in the spectra of mass-losing OB stars - Indications of corotating interaction regions? will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1290014