Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26a...302..169n&link_type=abstract
Astronomy and Astrophysics, v.302, p.169
Astronomy and Astrophysics
Astrophysics
52
Stars:Circumstellar Matter, Stars: Be, Stars: Mass-Loss, Stars: Pre-Main Sequence, Ism: Jets And Outflows, Infrared: Stars
Scientific paper
We present results of the observations of infrared HI recombination lines (namely Paβ, Brγ, Brα, Pfγ and Pfβ) from 14 Herbig Ae/Be stars. From line luminosities, and using an ionized wind model, we have determined the wind mass loss rates of these stars. The values obtained are in the range 10^-8^ to 10^-6^xMsun_/yr. For those stars for which ˙(M)_w_ has also been independently determined from CO observations, we find a reasonable agreement between the two estimates. We find a correlation between ˙(M)_w_ and the star's bolometric luminosity, which is in agreement with previous results for Young Stellar Objects (YSOs): a similar relation holds also for classical Be stars, although at a significantly lower level, suggesting a continuity of the mass loss mechanism during the evolution of intermediate mass stars. From the analysis of the correlation between mass loss rates and different indicators of the source stellar and circumstellar environment, we conclude that a proportionality between the mass loss rate and the stellar mass can account for the observed results.
Milillo Anna
Nisini Brunella
Saraceno Paolo
Vitali Fabio
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