TY - CONF
T1 - X-ray study of local infrared bright galaxies
AU - Pereira-Santaella, Miguel
AU - Alonso-Herrero, Almudena
AU - Jiménez-Bailón, Elena
AU - Rieke, George H.
AU - Santos-Lleo, María
AU - Ward, Martin
N1 - Funding Information:
This work is based on observations obtained with XMM-Newton, an ESA science mission with instruments and contributions directly funded by ESA Member States and the USA (NASA). MP-S acknowledges support from the CSIC under grant JAE-Predoc-2007. MP-S also thanks the Durham University for their hospitality during his stay while part of this work was done. AA-H and MP-S acknowledge support from the Spanish Plan Nacional del Espacio under grant ESP2007-65475-C02-01.
Funding Information:
acknowledge support from the Spanish Plan Nacional del Espacio under grant ESP2007-65475-C02-01.
Funding Information:
This work is based on observations obtained with XMM-Newton, an ESA science mission with instruments and contributions directly funded by ESA Member States and the USA (NASA). MP-S acknowledges support from the CSIC under grant JAE-Predoc-2007. MP-S also thanks the Durham University for their hospitality during his stay while part of this work was done. AA-H and MP-S
Publisher Copyright:
© 2020 Proceedings of the 9th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics VI, SEA 2010. All rights reserved.
PY - 2010/7/1
Y1 - 2010/7/1
N2 - We are carrying out detailed study of the X-ray and infrared (IR) properties of a sample of local (d < 70 Mpc) luminous infrared galaxies (LIRGs) using XMM-Newton and Spitzer (imaging and spectroscopy). The main goal is to study the extreme processes of star formation and/or active galactic nuclei (AGN) taking place in this cosmologically important class of galaxies. In this proceedings we present the preliminary results obtained from the analysis of the XMM-Newton X-ray images and the X-ray spectral modeling.
AB - We are carrying out detailed study of the X-ray and infrared (IR) properties of a sample of local (d < 70 Mpc) luminous infrared galaxies (LIRGs) using XMM-Newton and Spitzer (imaging and spectroscopy). The main goal is to study the extreme processes of star formation and/or active galactic nuclei (AGN) taking place in this cosmologically important class of galaxies. In this proceedings we present the preliminary results obtained from the analysis of the XMM-Newton X-ray images and the X-ray spectral modeling.
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M3 - Paper
AN - SCOPUS:85090696036
SP - 601
EP - 606
T2 - 9th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics VI, SEA 2010
Y2 - 13 September 2010 through 17 September 2010
ER -