65 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Consejo Nacional de Investigaciones Científicas y TécnicasAR17 papers
- Universidad Complutense de MadridES12 papers
- Universidad Nacional de La PlataAR12 papers
- Bariloche Atomic CentreAR8 papers
- Instituto Argentino de RadioastronomíaAR8 papers
- Osservatorio Astronomico di PalermoIT8 papers
- Universidad de JaénES7 papers
- Balseiro InstituteAR5 papers
- Comisión Nacional de Energía AtómicaAR3 papers
- National Institute for AstrophysicsIT3 papers
- University of PalermoIT3 papers
- Institute of Astronomy and Space PhysicsAR2 papers
4 papers · 1 filter
X-ray emission from massive stars in Cyg OB2
G. Rauw, Y. Naze, N. J. Wright +9
We report on the analysis of the Chandra-ACIS data of O, B and WR stars in the young association Cyg OB2. X-ray spectra of 49 O-stars, 54 B-stars and 3 WR-stars are analyzed and fo…
A comprehensive study of NGC 2023 with XMM-Newton and Spitzer
M. A. López-García, J. López-Santiago, J. F. Albacete-Colombo +2
Nearby star-forming regions are ideal laboratories to study high-energy emission of different stellar populations, from very massive stars to brown dwarfs. NGC 2023 is a reflection…
Deep XMM-Newton observation of the Eta Chamaleontis cluster
J. Lopez-Santiago, J. F. Albacete Colombo, M. A. Lopez-Garcia
The members of the Eta Chamaleontis cluster are in an evolutionary stage in which disks are rapidly evolving. It also presents some peculiarities, such as the large fraction of bin…
HRC-I/Chandra X-ray observations towards sigma Orionis
J. A. Caballero, J. F. Albacete-Colombo, J. Lopez-Santiago
Aims: We investigated the X-ray emission from young stars and brown dwarfs in the sigma Orionis cluster (tau~3 Ma, d~385 pc) and its relation to mass, presence of circumstellar dis…