Achim Feldmeier
Achim Feldmeier
apl Professor, Universität Potsdam
Verified email at - Homepage
Cited by
Cited by
O-star mass-loss and wind momentum rates in the Galaxy and the Magellanic Clouds Observations and theoretical predictions.
J Puls, RP Kudritzki, A Herrero, AWA Pauldrach, SM Haser, DJ Lennon, ...
Astronomy and Astrophysics, v. 305, p. 171 305, 171, 1996
A possible origin for X-rays from O stars.
A Feldmeier, J Puls, AWA Pauldrach
Astronomy and Astrophysics, v. 322, p. 878-895 322, 878-895, 1997
Neglecting the porosity of hot-star winds can lead to underestimating mass-loss rates
LM Oskinova, WR Hamann, A Feldmeier
Astronomy & Astrophysics 476 (3), 1331-1340, 2007
Time-dependent structure and energy transfer in hot star winds.
A Feldmeier
Astronomy and Astrophysics, v. 299, p. 523 299, 523, 1995
The IUE Mega Campaign: Wind variability and rotation in early-type stars
D Massa, AW Fullerton, JS Nichols, SP Owocki, RK Prinja, N St-Louis, ...
The Astrophysical Journal 452 (1), L53, 1995
High-resolution X-ray spectroscopy of bright O-type stars
LM Oskinova, A Feldmeier, WR Hamann
Monthly Notices of the Royal Astronomical Society 372 (1), 313-326, 2006
The X-ray emission from shock cooling zones in O star winds.
A Feldmeier, RP Kudritzki, R Palsa, AWA Pauldrach, J Puls
Astronomy and Astrophysics, v. 320, p. 899-912 320, 899-912, 1997
Mass loss from inhomogeneous hot star winds-I. Resonance line formation in 2D models
JO Sundqvist, J Puls, A Feldmeier
Astronomy & Astrophysics 510, A11, 2010
X-ray line emission from a fragmented stellar wind
A Feldmeier, L Oskinova, WR Hamann
Astronomy & Astrophysics 403 (1), 217-224, 2003
Mass loss from inhomogeneous hot star winds-II. Constraints from a combined optical/UV study
JO Sundqvist, J Puls, A Feldmeier, SP Owocki
Astronomy & Astrophysics 528, A64, 2011
Clumped stellar winds in supergiant high‐mass X‐ray binaries: X‐ray variability and photoionization
LM Oskinova, A Feldmeier, P Kretschmar
Monthly Notices of the Royal Astronomical Society 421 (4), 2820-2831, 2012
Three-dimensional radiative transfer in clumped hot star winds-I. Influence of clumping on the resonance line formation
B Šurlan, WR Hamann, J Kubát, LM Oskinova, A Feldmeier
Astronomy & Astrophysics 541, A37, 2012
X-ray emission lines from inhomogeneous stellar winds
LM Oskinova, A Feldmeier, WR Hamann
Astronomy & Astrophysics 422 (2), 675-691, 2004
Clumping in Hot Star Winds: Proceedings of an International Workshop Held in Potsdam, Germany, 18.-22. June 2007
WR Hamann
Universitätsverlag Potsdam, 2008
Discovery of X-ray emission from the Wolf–Rayet star WR 142 of oxygen subtype
LM Oskinova, WR Hamann, A Feldmeier, R Ignace, YH Chu
The Astrophysical Journal 693 (1), L44, 2009
Clumpy wind accretion in supergiant neutron star high mass X-ray binaries
E Bozzo, L Oskinova, A Feldmeier, M Falanga
Astronomy & Astrophysics 589, A102, 2016
Dynamics of Line-driven Winds from Disks in Cataclysmic Variables. I. Solution Topology and Wind Geometry
A Feldmeier, I Shlosman
The Astrophysical Journal 526 (1), 344, 1999
Time-dependent modeling of extended thin decretion disks of critically rotating stars
P Kurfürst, A Feldmeier, J Krtička
Astronomy & Astrophysics 569, A23, 2014
VELA X-1: how to produce asymmetric eclipses.
A Feldmeier, U Anzer, G Boerner, F Nagase
Astronomy and Astrophysics, v. 311, p. 793-802 311, 793-802, 1996
Radiation driven winds of hot stars: Theory of O-star atmospheres as a spectroscopic tool
AWA Pauldrach, A Feldmeier, J Puls, RP Kudritzki
Space Science Reviews 66, 105-125, 1993
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