Revisited mass-loss rates for the nuclei of the planetary nebulae NGC 6210, NGC 6826 and NGC 6543 - The first order moment W1 of subordinate line profiles

Details Revisited mass-loss rates for the nuclei of the planetary nebulae NGC 6210, NGC 6826 and NGC 6543 - The first order moment W1 of subordinate line profiles Revisited mass-loss rates for the nuclei of the planetary nebulae NGC 6210, NGC 6826 and NGC 6543 - The first order moment W1 of subordinate line profiles

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...173..101h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 173, no. 1, Feb. 1987, p. 101-107.

Statistics

Computation

10

B Stars, Line Shape, Mass Flow Rate, Planetary Nebulae, Stellar Envelopes, Stellar Mass Ejection, Abundance, Computational Astrophysics, Cygnus Constellation, Nuclei, Optical Thickness, Velocity Distribution

Scientific paper

The authors present the results of numerical calculations for the first order moment W1 of subordinate P Cygni line profiles as a function of the parameter W10αM>ngngng