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Results 1 - 13 of 13
First detection of bromine and antimony in hot stars★★★
Volume 13, Issue 25 - article #9
K. Werner
,
T. Rauch
,
M. Knörzer
,
J. W. Kruk
Astronomy & Astrophysics
http://feedproxy.google.com/~r/edp_aa/~3/PqkUe8I3NoA/201832723
Stellar laboratories - III. New Ba v, Ba vi, and Ba vii oscillator strengths and the barium abundance in the hot white dwarfs G191−B2B and RE 0503–289
Volume 9, Issue 21 - article #48
T. Rauch
,
K. Werner
,
P. Quinet
and
J. W. Kruk
Astronomy and Astrophysics - Volume: 566, Issue: June 2014
http://dx.doi.org/10.1051/0004-6361/201423878
Abstract
Full HTML
PDF (242.7 KB)
ePUB (1.625 MB)
References
Tables at CDS
NASA ADS Abstract Service
Stellar laboratories III. New Ba V, Ba VI, and Ba VII oscillator strengths and the barium abundance in the hot white dwarfs G191-B2B and RE0503-289
Volume 9, Issue 17 - article #7
T. Rauch
(1),
K. Werner
(1),
P. Quinet
(2,3),
J. W. Kruk
(4)
((1) Institute for Astronomy and Astrophysics, Eberhard Karls University, Tuebingen, Germany,
(2) Astrophysique et Spectroscopie, Universite de Mons - UMONS, Belgium,
(3) IPNAS, Universite de Liege, Liege, Belgium,
(4) NASA Goddard Space Flight Center, Greenbelt, USA)
arXiv.org - Astrophysics - Volume: 2014, Issue: 25 Apr
arXiv:1404.6094
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The virtual observatory service TheoSSA: Establishing a database of synthetic stellar flux standards. I. NLTE spectral analysis of the DA-type white dwarf G 191-B2B
Volume 8, Issue 35 - article #13
T. Rauch
(1),
R. Bohlin
(2),
J. W. Kruk
(3),
K. Werner
(1)
((1) Institute for Astronomy and Astrophysics, Kepler Center for Astro and Particle Physics, Eberhard Karls University, Tuebingen, Germany,
(2) Space Telescope Science Institute, Baltimore, MD, USA,
(3) NASA Goddard Space Flight Center, Greenbelt, MD, USA)
arXiv.org - Astrophysics - Volume: 2013, Issue: 30 Aug
arXiv:1308.6450
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Metal Abundances in Hot DO White Dwarfs
Volume 7, Issue 39 - article #15
K. Werner
,
T. Rauch
,
E. Ringat
,
J. W. Kruk
arXiv.org - Astrophysics - Volume: 2012, Issue: 28 Sep
arXiv:1209.4977
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Discovery of Iron in PG1159 Stars
Volume 5, Issue 52 - article #3
K. Werner
,
T. Rauch
,
J. W. Kruk
arXiv.org - Astrophysics - Volume: 2010, Issue: 24 Dec
arXiv:1012.5228
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Virtual Observatory studies of Planetary Nebulae
Volume 4, Issue 6 - article #17
R. P. Mignani
(MSSL-UCL),
F. Kerber
(ESO),
R. L. Smart
(INAF),
D. Vande Putte
(MSSL-UCL),
A. Wicenec
(ESO),
T. Rauch
(U.Tubingen),
H.M. Adorf
(MPA),
R. Harrison
(Rosebury School)
arXiv.org - Astrophysics - Volume: 2009, Issue: 5 Feb
arXiv:0902.0960
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Discovery of photospheric Ca X emission lines in the far-UV spectrum of the hottest known white dwarf (KPD 0005+5106)
Volume 3, Issue 50 - article #19
K. Werner
,
T. Rauch
,
and
J. W. Kruk
Astronomy and Astrophysics - Volume: 492, Issue: 3
Abstract
|
PDF file (141.7 KB)
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PS file (88.37 KB)
Elemental Abundances in PG1159 Stars
Volume 2, Issue 43 - article #8
K. Werner
,
T. Rauch
,
E. Reiff
,
J.W. Kruk
arXiv.org - Astrophysics - Volume: 2007, Issue: 25 Oct
arXiv:0710.4506
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KPD0005+5106: Hottest DO White Dwarf Much Hotter Than Assumed
Volume 2, Issue 43 - article #12
K. Werner
,
T. Rauch
,
J. W. Kruk
arXiv.org - Astrophysics - Volume: 2007, Issue: 25 Oct
arXiv:0710.4515
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Discovery of photospheric argon in very hot central stars of planetary nebulae and white dwarfs
Volume 2, Issue 7 - article #13
K. Werner
,
T. Rauch
,
J.W. Kruk
ArXiv - Astrophysics
astro-ph/0702387 [
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pdf
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other
]
Spectral analyses of 16 DAO white dwarfs from the Sloan Digital Sky Survey
Volume 1, Issue 39 - article #16
S. D. Huegelmeyer
(1),
S. Dreizler
(1),
T. Rauch
(2),
J. Krzesinski
(3)
((1) Institut fuer Astrophysik, Goettingen, Germany,
(2) Institut fuer Astronomie und Astrophysik, Tuebingen, Germany,
(3) Apache Point Observatory, New Mexico State University, USA)
ArXiv - Astrophysics
astro-ph/0610744 [
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other
]
AGB star intershell abundances inferred from analyses of extremely hot H-deficient post-AGB stars
Volume 1, Issue 7 - article #19
K. Werner
,
D. Jahn
,
T. Rauch
,
E. Reiff
,
F. Herwig
,
J.W. Kruk
ArXiv - Astrophysics
astro-ph/0603225 [
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]
Results 1 - 13 of 13
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