Astronomers link space explosion to huge, mysterious star -...
www.csmonitor.com
The progenitor of supernova SN 2013cu was a nitrogen-rich Wolf-Rayet star, say astronomers using a new technique to identify the chemistry of stars just after...
abstract
www.astro.physik.uni-potsdam.de
XMM-Newton Observations of the Nitrogen-Rich Wolf-Rayet star WR1 R. Ignace 1, L. Oskinova 2 and J. C. Brown 3 University of Wisconsin, USA 1; University of Potsdam ...
publish.UP Dust formation in carbon-rich Wolf-Rayet colliding winds
publishup.uni-potsdam.de
Carbon-rich Wolf-Rayet stars are efficient carbon dust makers. Despite the strong evidence for dust formation in these objects provided by infrared thermal...
XMM-Newton observations of the nitrogen-rich Wolf-Rayet star WR
eprints.gla.ac.uk
XMM-Newton observations of the nitrogen-rich Wolf-Rayet star WR 1. Ignace, R., Oskinova, L.M., and Brown, J.C. (2003) XMM-Newton ...
Are luminous and metal-rich Wolf Rayet stars inflated?
dspace.library.uu.nl
Aims. We investigate the influence of metallicity and stellar wind mass loss on the radius of Wolf-Rayet stars. Methods. We have calculated chemically ...
Astrophysics and Space Science: Volume 255, An...
books.google.de
These stellar winds have a profound effect on the evolution of the most massive stars, e.g. they lead to the formation of He-rich Wolf-Rayet (WR) stars.
The Infrared Spectral Region of Stars - Google Books
books.google.de
THE INFRARED SPECTRUM OF THE OXYGEN-RICH WOLF-RAYET STAR ST3 P.R. EENENS(1) - P.M. WILLIAMS(2) Department of Astronomy, University of ...
Are luminous and metal-rich Wolf-Rayet stars inflated? - NASA/ADS
ui.adsabs.harvard.edu
Results: .We confirm the radius extension for luminous, metal-rich Wolf-Rayet stars reported previously by Ishii et al. (1999, PASJ, 51, 417), i.e. the inflation of the ...
ASTRONOMY AND ISO-SWS observations of infrared absorption …
aa.springer.de
ISO-SWS observations of infrared absorption bands of the diffuse interstellar medium: The 6.2 m feature of aromatic compounds? ... C-rich Wolf-Rayet stars.
Wolf-Rayet stars and OB assoctations as gamma-ray...
aa.springer.de
to three possible origins: carbon rich Wolf-Rayet (W-R) stars, supernovae with massive progenitors (˘ 60M
Alle Infos zum Namen "Rich Wolf"
(PDF) Dust Formation Chemistry in Carbon-Rich Wolf-Rayet Winds |...
www.academia.edu
wind of carbon-rich Wolf-Rayet (WC) stars. Results show that dust precursors ...
Dust Formation Chemistry in Carbon Rich Wolf Rayet Winds - Technische...
www.tib.eu
Dust Formation Chemistry in Carbon-Rich Wolf-Rayet Winds (P). Author / Creator : Le Tueff, Y. H. ; Cherchneff, I. ; UMIST. In: ASTROPHYSICS AND SPACE ...
Are luminous and metal-rich Wolf-Rayet stars inflated? | Astronomy &...
www.aanda.org
Results.We confirm the radius extension for luminous, metal-rich Wolf-Rayet stars reported previously by Ishii et al. (1999, PASJ, 51, 417), i.e. the inflation of the ...
XMM-Newton observations of the nitrogen-rich Wolf-Rayet star WR 1 |...
www.aanda.org
We present XMM-Newton results for the X-ray spectrum from the N-rich Wolf-Rayet (WR) star WR 1. The EPIC instrument was used to obtain a ...
wo - abbreviation: wo - all meanings
abbreviations.woxikon.com
(celestial object) Oxygen-rich Wolf-Rayet, a Wolf-Rayet star with strong oxygen spectral line emission : astronomy : WO ...
"XMM-Newton observations of the nitrogen-rich Wolf-Rayet star WR 1."...
works.bepress.com
Berkeley Electronic Press Selected Works
MOST finds no coherent oscillations in the hot carbon-rich Wolf-Rayet...
library2.smu.ca
We have photometrically monitored the V = 8 mag Galactic Population I WC5 star WR 111 for 3 weeks nonstop using the MOST microsatellite. Each of the ...
New Supernova Likely Arose From Massive Wolf-Rayet Star - Universe...
www.universetoday.com
They've been identified as possible causes for supernovae for a while, but until now, there was a lack of evidence linking massive Wolf-Rayet stars to thes
MOST Finds No Coherent Oscillations in the Hot Carbon-rich Wolf-Rayet...
ucris.univie.ac.at
MOST Finds No Coherent Oscillations in the Hot Carbon-rich Wolf-Rayet Star HD (WR 111). Veröffentlichung: Beitrag in Fachzeitschrift › Artikel.
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