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19992023
most citedMass loss from hot massive stars

644 citations · 7.3k across the 88 of their papers we have counts for

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astro-ph2008★ 644 cited

Mass loss from hot massive stars

J. Puls, J. S. Vink, F. Najarro

Mass loss is a key process in the evolution of massive stars, and must be understood quantitatively to be successfully included in broader astrophysical applications. In this revie…

astro-ph2008★ 91 cited

The Physical Properties and Effective Temperature Scale of O-type Stars as a Function of Metallicity. III. More Results from the Magellanic Clouds

Philip Massey, Amanda M. Zangari, Nidia I. Morrell +4

In order to better determine the physical properties of hot, massive stars as a function of metallicity, we obtained very high SNR optical spectra of 26 O and early B stars in the…

astro-ph2007★ 176 cited

Bright OB stars in the Galaxy IV. Stellar and wind parameters of early to late B supergiants

N. Markova, J. Puls

We apply the NLTE atmosphere code FASTWIND to perform a spectroscopic study of a small sample of Galactic B-supergiants from B0 to B9. By means of the resulting data and incorporat…

astro-ph2007★ 317 cited

The empirical metallicity dependence of the mass-loss rate of O- and early B-type stars

M. R. Mokiem, A. de Koter, J. S. Vink +9

[Abridged] We present a comprehensive study of the metallicity dependence of the mass-loss rates in stationary stellar winds of hot massive stars. Assuming a power-law dependence o…

astro-ph2007★ 78 cited

Towards an understanding of the Of?p star HD 191612: optical spectroscopy

Ian D. Howarth, Nolan R. Walborn, Danny J. Lennon +17

We present extensive optical spectroscopy of the early-type magnetic star HD 191612 (O6.5f?pe-O8fp). The Balmer and HeI lines show strongly variable emission which is highly reprod…

astro-ph2007★ 168 cited

The VLT-FLAMES survey of massive stars: Wind properties and evolution of hot massive stars in the LMC

M. R. Mokiem, A. de Koter, C. J. Evans +9

[Abridged] We have studied the optical spectra of 28 O- and early B-type stars in the Large Magellanic Cloud, 22 of which are associated with the young star-forming region N11. Ste…