[HTML][HTML] The 0.1-2.5-KEV X-Ray Spectrum of the O4F-STAR Zeta-Puppis

DJ Hillier, RP Kudritzki, AW Pauldrach… - … , Vol. 276, NO. 1 …, 1993 - adsabs.harvard.edu
We have obtained a high quality ROSAT PSPC spectrum of the bright O4f star ζ Pup.
Allowing for the wind X-ray opacity, as computed from detailed non-LTE stellar wind models …

The 0.1-2.5 keV X-ray spectrum of the O4f star dzeta Puppis.

DJ Hillier, RP Kudritzki, AW Pauldrach… - Astronomy and …, 1993 - ui.adsabs.harvard.edu
We have obtained a high quality ROSAT PSPC spectrum of the bright O4f star ζ Pup.
Allowing for the wind X-ray opacity, as computed from detailed non-LTE stellar wind models …

[PDF][PDF] The 0.1-2.5 keV X-ray spectrum of the O4f star (Puppis

DJ Hillier, RP Kudritzki, AW Pauldrach, D Baade… - Astron …, 1993 - researchgate.net
We have obtained a high quality ROSAT PSPC spectrum of the bright O4f star Ç Pup.
Allowing for the wind X-ray opacity, as computed from detailed non-LTE stellar wind models …

[引用][C] The 0.1-2.5 keV X-ray spectrum of the O4f star ζ Puppis

DJ HILLIER, RP KUDRITZKI… - Astronomy and …, 1993 - pascal-francis.inist.fr
The 0.1-2.5 keV X-ray spectrum of the O4f star ζ Puppis CNRS Inist Pascal-Francis CNRS
Pascal and Francis Bibliographic Databases Simple search Advanced search Search by …

[PDF][PDF] The 0.1-2.5 keV X-ray spectrum of the 04f star£ Puppis

DJ Hillier, RP Kudritzki, AW Pauldrach… - Astron …, 1993 - usm.uni-muenchen.de
We have obtained a high quality ROSAT PSPC spectrum of the bright 04 f star£ Pup.
Allowing for the wind X-ray opacity, as computed from detailed non-LTE stellar wind models …

[PDF][PDF] The 0.1-2.5 keV X-ray spectrum of the O4f star (Puppis

DJ Hillier, RP Kudritzki, AW Pauldrach… - Astron …, 1993 - usm.uni-muenchen.de
We have obtained a high quality ROSAT PSPC spectrum of the bright O4f star Ç Pup.
Allowing for the wind X-ray opacity, as computed from detailed non-LTE stellar wind models …