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08 May 2024
 
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Results 1 to 20 of 21 for query "Lidia Oskinova". (0.01 sec.)

[    1    2    ]   Next

1.
X-raying the super star clusters in the Galactic center
L.M. Oskinova;
29 Jul 2005
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2.
Evolution of X-ray emission from young massive star clusters
L.M. Oskinova;
25 May 2005   /  Mon.Not.Roy.Astron.Soc. 361 (2005) 679-694
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3.
X-ray emission lines from inhomogeneous stellar winds
L.M. Oskinova; A. Feldmeier; W.-R. Hamann;
31 Mar 2004   /  Astron.Astrophys. 422 (2004) 675-691
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4.
The Conspicuous Absence of X-ray Emission from Carbon-Enriched Wolf-Rayet Stars
L.M.Oskinova; R.Ignace; W.-R. Hamann; A.M.T.Pollock; J.C.Brown;
3 Mar 2003   /  Astron.Astrophys. 402 (2003) 755-766
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5.
Modelling X-ray variability in the structured atmospheres of hot stars
L. M. Oskinova; R. Ignace; J. C. Brown; J. P. Cassinelli;
25 Apr 2001
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6.
Ionization of HeII in star-forming galaxies by X-rays from cluster winds and superbubbles
Lidia Oskinova; Daniel Schaerer;
9 Mar 2022
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7.
A Deep Exposure in High Resolution X-Rays Reveals the Hottest Plasma in the $zeta,$Puppis Wind
David P. Huenemoerder; Richard Ignace; Nathan A. Miller; Kenneth G. Gayley; Wolf-Rainer Hamann; Jennifer Lauer; Anthony F.J. Moffat; Yaël Nazé; Joy S. Nichols; Lidia Oskinova; Noel D. Richardson; Wayne Waldron;
15 Mar 2020
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8.
Probing Wolf-Rayet Winds: Chandra/HETG X-Ray Spectra of WR 6
David P. Huenemoerder; Kenneth G. Gayley; Wolf-Rainer Hamann; Richard Ignace; Joy S. Nichols; Lidia Oskinova; Andrew M. T. Pollock; Norbert S. Schulz; Tomer Shenar;
5 Nov 2015
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9.
A Report on the X-ray Properties of the tau Sco Like Stars
Richard Ignace; Lidia Oskinova; Derck Mass;
5 Nov 2012
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10.
3-D Monte Carlo radiative transfer calculation of resonance line formation in the inhomogeneous expanding stellar wind
Brankica Šurlan; Wolf-Rainer Hamann; Jiří Kubát; Lidia Oskinova; Achim Feldmeier;
21 Feb 2012
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11.
X-rays, clumping and stellar wind structures
Lidia Oskinova; Wolf-Rainer Hamann; Richard Ignace; Achim Feldmeier;
8 Dec 2010
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12.
The excess of cool supergiants from contemporary stellar evolution models defies the metallicity-independent Humphreys-Davidson limit
Avishai Gilkis; Tomer Shenar; Varsha Ramachandran; Adam S. Jermyn; Laurent Mahy; Lidia M. Oskinova; Iair Arcavi; Hugues Sana;
5 Feb 2021
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13.
Chandra's X-ray study confirms that the magnetic standard Ap star KQ Vel hosts a neutron star companion
Lidia M. Oskinova; Richard Ignace; Paolo Leto; Konstantin A. Postnov;
22 Jul 2020
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14.
Coupling hydrodynamics with comoving frame radiative transfer: II. Stellar wind stratification in the high-mass X-ray binary Vela X-1
Andreas A.C. Sander; Felix Fürst; Peter Kretschmar; Lidia M. Oskinova; Helge Todt; Rainer Hainich; Tomer Shenar; Wolf-Rainer Hamann;
9 Aug 2017
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15.
Stellar Winds in Massive X-ray Binaries
Peter Kretschmar; Silvia Martínez-Núñez; Enrico Bozzo; Lidia M. Oskinova; Joachim Puls; Lara Sidoli; Jon Olof Sundqvist; Pere Blay; Maurizio Falanga; Felix Fürst; Angel Gímenez-García; Ingo Kreykenbohm; Matthias Kühnel; Andreas Sander; José Miguel Torrejón; Jörn Wilms; Philipp Podsiadlowski; Antonios Manousakis;
22 Feb 2017
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16.
Towards a unified view of inhomogeneous stellar winds in isolated supergiant stars and supergiant high mass X-ray binaries
Silvia Martínez-Núñez; Peter Kretschmar; Enrico Bozzo; Lidia M. Oskinova; Joachim Puls; Lara Sidoli; Jon Olof Sundqvist; Pere Blay; Maurizio Falanga; Felix Fürst; Ángel Gímenez-García; Ingo Kreykenbohm; Matthias Kühnel; Andreas Sander; José Miguel Torrejón; Jörn Wilms;
30 Jan 2017
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17.
Moving inhomogeneous envelopes of stars
Lidia M. Oskinova; Brankica Kubatova; Wolf-Rainer Hamann;
8 Jul 2016
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18.
A detailed X-ray investigation of zeta Puppis - The variability on short and long timescales
Yael Naze; Lidia M. Oskinova; Eric Gosset;
7 Dec 2012
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19.
On the Weak-Wind Problem in Massive Stars: X-ray Spectra Reveal a Massive Hot Wind in mu Columbae
David P. Huenemoerder; Lidia M. Oskinova; Richard Ignace; Wayne L. Waldron; Helge Todt; Kenji Hamaguchi; Shunji Kitamoto;
3 Aug 2012
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20.
3-D radiative transfer in clumped hot star winds I. Influence of clumping on the resonance line formation
Brankica Šurlan; Wolf-Rainer Hamann; Jiří Kubát; Lidia M. Oskinova; Achim Feldmeier;
21 Feb 2012
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