Home

About

Advanced Search

Browse by Discipline

Scientific Societies

E-print Alerts

Add E-prints

E-print Network
FAQHELPSITE MAPCONTACT US


  Advanced Search  

 
SOME LIKE IT HOT: THE X-RAY EMISSION OF THE GIANT STAR YY MENSAE Marc Audard
 

Summary: SOME LIKE IT HOT: THE X-RAY EMISSION OF THE GIANT STAR YY MENSAE
Marc Audard
Columbia Astrophysics Laboratory, Mail Code 5247, 550 West 120th Street,
New York, NY 10027; audard@astro.columbia.edu
Alessandra Telleschi and Manuel Gu¨del
Paul Scherrer Institut, Wu¨renlingen und Villigen, 5232 Villigen PSI, Switzerland;
atellesc@astro.phys.ethz.ch, guedel@astro.phys.ethz.ch
Stephen L. Skinner
Center for Astrophysics and Space Astronomy, University of Colorado, Boulder,
CO 80309-0389; skinners@casa.colorado.edu
Roberto Pallavicini
Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, 90134
Palermo, Italy; pallavic@oapa.astropa.unipa.it
and
Urmila Mitra-Kraev
Mullard Space Science Laboratory, University College London, Holmbury St. Mary,
Dorking, Surrey RH5 6NT, UK; umk@mssl.ucl.ac.uk
Receivved 2004 May 5; accepted 2004 July 16
ABSTRACT
We present an analysis of the X-ray emission of the rapidly rotating giant star YY Mensae observed by Chandra

  

Source: Audard, Marc - INTEGRAL Science Data Centre & Observatory of Geneva, Université de Genève

 

Collections: Physics