Franz Kerschbaum
Franz Kerschbaum
Department of Astrophysics, University of Vienna, Austria
Email verificata su - Home page
Citata da
Citata da
The Herschel Photodetector Array Camera & Spectrometer (PACS): design and in-flight operation and scientific performance
A Poglitsch, C Waelkens, OH Bauer, J Cepa, H Feuchtgruber, T Henning, ...
cosp 38, 13, 2010
The photodetector array camera and spectrometer (PACS) on the Herschel space observatory
A Poglitsch, C Waelkens, N Geis, H Feuchtgruber, B Vandenbussche, ...
Astronomy & astrophysics 518, L2, 2010
A far-infrared survey of bow shocks and detached shells around AGB stars and red supergiants
NLJ Cox, F Kerschbaum, AJ van Marle, L Decin, D Ladjal, A Mayer, ...
Astronomy & Astrophysics 537, A35, 2012
Mass loss rates of a sample of irregular and semiregular M-type AGB-variables
H Olofsson, DG Delgado, F Kerschbaum, FL Schier
Astronomy & Astrophysics 391 (3), 1053-1067, 2002
Dust shells around carbon Mira variables
MAT Groenewegen, PA Whitelock, CH Smith, F Kerschbaum
Monthly Notices of the Royal Astronomical Society 293 (1), 18-42, 1998
Unexpectedly large mass loss during the thermal pulse cycle of the red giant star R Sculptoris
M Maercker, S Mohamed, WHT Vlemmings, S Ramstedt, ...
Nature 490 (7419), 232-234, 2012
On the origin of the 13 mu m feature. A study of ISO-SWS spectra of oxygen-rich AGB stars
T Posch, F Kerschbaum, H Mutschke, D Fabian, J Dorschner, J Hron
Astronomy and Astrophysics 352, 609-618, 1999
Semiregular variables of types sra and srb-basic properties in the visual and the iras-range
F Kerschbaum, J Hron
Astronomy and Astrophysics 263, 97-112, 1992
MESS (Mass-loss of Evolved StarS), a Herschel key program
MAT Groenewegen, C Waelkens, MJ Barlow, F Kerschbaum, ...
Astronomy & Astrophysics 526, A162, 2011
“Thermal” SiO radio line emission towards M-type AGB stars: A probe of circumstellar dust formation and dynamics
DG Delgado, H Olofsson, F Kerschbaum, FL Schier, M Lindqvist, ...
Astronomy & Astrophysics 411 (2), 123-147, 2003
Semiregular variables of types SRa and SRb. New JHKL'M-photometry for 200 stars.
F Kerschbaum, J Hron
Astronomy and Astrophysics Supplement Series 106, 397-411, 1994
Near-infrared photometry of a sample of IRAS point sources
P Fouqu, T Le Bertre, N Epchtein, F Guglielmo, F Kerschbaum
Astronomy and Astrophysics Supplement Series 93, 151-171, 1992
Infrared optical properties of spinels-A study of the carrier of the 13, 17 and 32 μm emission features observed in ISO-SWS spectra of oxygen-rich AGB stars
D Fabian, T Posch, H Mutschke, F Kerschbaum, J Dorschner
Astronomy & Astrophysics 373 (3), 1125-1138, 2001
Warm water vapour in the sooty outflow from a luminous carbon star
L Decin, M Agndez, MJ Barlow, F Daniel, J Cernicharo, R Lombaert, ...
Nature 467 (7311), 64-67, 2010
Oxygen-rich semiregular and irregular variables-A catalogue of circumstellar CO observations
F Kerschbaum, H Olofsson
Astronomy and Astrophysics Supplement Series 138 (2), 299-322, 1999
Identification of 106 new infrared carbon stars in the IRAS Point Source Catalog-Near-infrared photometry and their space distribution in the galaxy
F Guglielmo, N Epchtein, T Le Bertre, P Fouque, J Hron, F Kerschbaum, ...
Astronomy and Astrophysics Supplement Series 99, 31-69, 1993
The enigmatic nature of the circumstellar envelope and bow shock surrounding Betelgeuse as revealed by Herschel-I. Evidence of clumps, multiple arcs, and a linear bar-like…
L Decin, NLJ Cox, P Royer, AJ Van Marle, B Vandenbussche, D Ladjal, ...
Astronomy & Astrophysics 548, A113, 2012
On the origin of the 19.5 m feature-Identifying circumstellar Mg-Fe-oxides
T Posch, F Kerschbaum, H Mutschke, J Dorschner, C Jger
Astronomy & Astrophysics 393 (1), L7-L10, 2002
Long period variables detected by ISO in the Small Magellanic Cloud
MRL Cioni, J Blommaert, MAT Groenewegen, HJ Habing, J Hron, ...
Astronomy & Astrophysics 406 (1), 51-63, 2003
Semiregular variables of types SRa and SRb. Energy distributions and stellar parameters.
F Kerschbaum, J Hron
Astronomy and Astrophysics 308, 489-496, 1996
Il sistema al momento non pu eseguire l'operazione. Riprova pi tardi.
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