24 citations · 28 across the 3 of their papers we have counts for
3 papers
astro-ph.SR2010
A proper description of clumping in hot star winds: the key to obtaining reliable mass-loss rates?
Jon O. Sundqvist, Joachim Puls, Achim Feldmeier +1
Small-scale inhomogeneities, or `clumping', in the winds of hot, massive stars are conventionally included in spectral analyses by assuming optically thin clumps. To reconcile inve…
astro-ph.SR2009★ 4 cited
Mass loss from OB-stars
J. Puls, J. O. Sundqvist, F. Najarro +1
We review recent developments regarding radiation driven mass loss from OB-stars. We first summarize the fundamental theoretical predictions, and then compare these to observationa…
astro-ph2008★ 24 cited
Mg I emission lines at 12 and 18 micrometer in K giants
J. O. Sundqvist, N. Ryde, G. M. Harper +2
The solar Mg I emission lines at 12 micrometer have already been observed and analyzed well. Previous modeling attempts for other stars have, however, been made only for Procyon an…