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Mass Loss Rates from B[e] Stars
1998Mass loss rates for a sample of eight blue supergiants are calculated using the hydrogen lines Hα, Hβ and Pδ. B[e] stars have a M vs L relationship flatter than that of OB stars, and mass loss rates comparable to those observed in WR stars.
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Mass loss rate of the zodiacal dust cloud
The Moon and the Planets, 1983The mass loss rate of the zodiacal dust cloud near the Sun has been estimated on the basis of the orbital behaviour of circumsolar dust grains suffering sublimation. It is found that the solar dust ring located at 4 solar radii from the Sun, which consists of grains whose inward spiraling due to the Poynting-Robertson effect is stopped by the influence
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Quantitative Results on AGB Mass-Loss Rates
2007We present new mass-loss rates for AGB stars derived from fitting circumstellar dust models to the spectral energy distributions from 1 to 35 mum of 26 LMC stars and 14 SMC stars. It is found that for pulsation periods greater than 500 days, there is a very tight correlation of mass-loss rate with pulsation period, but for shorter periods there is a ...
Wood, P.R. +17 more
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Colorectal cancer statistics, 2020
Ca-A Cancer Journal for Clinicians, 2020Rebecca L Siegel +2 more
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American Cancer Society nutrition and physical activity guideline for cancer survivors
Ca-A Cancer Journal for Clinicians, 2022Cheryl L Rock +2 more
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