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The excitation mechanisms of X-ray oxygen emission-lines

Published online by Cambridge University Press:  29 March 2021

Victoria Reynaldi Open the ORCID record for Victoria Reynaldi [Opens in a new window] ,
Matteo Guainazzi ,
Stefano Bianchi ,
Ileana Andruchow ,
Federico García ,
Iván López  and
Nicolás Salerno
Victoria Reynaldi
Affiliation:
Facultad de Ciencias Astronómicas y Geofísicas - Universidad Nacional de La Plata Paseo del Bosque s/n. La Plata, Argentina email: [email protected]
Matteo Guainazzi
Affiliation:
ESA/European Space Technology and Research Centre (ESTEC) D-SRE, Keplerlaan 1, 2200 AG, Noordwijk, The Netherlands
Stefano Bianchi
Affiliation:
Dipartimento di Matematica e Fisica, Università degli Studi Roma Tre via della Vasca Navale 84, I-00146 Roma, Italy
Ileana Andruchow
Affiliation:
Facultad de Ciencias Astronómicas y Geofísicas - Universidad Nacional de La Plata Paseo del Bosque s/n. La Plata, Argentina email: [email protected] Instituto de Astrofísica de La Plata, Paseo del Bosque s/n. La Plata, Argentina
Federico García
Affiliation:
Facultad de Ciencias Astronómicas y Geofísicas - Universidad Nacional de La Plata Paseo del Bosque s/n. La Plata, Argentina email: [email protected] Kapteyn Astronomical Institute, University of Groningen, The Netherlands
Iván López
Affiliation:
Facultad de Ciencias Astronómicas y Geofísicas - Universidad Nacional de La Plata Paseo del Bosque s/n. La Plata, Argentina email: [email protected]
Nicolás Salerno
Affiliation:
Facultad de Ciencias Astronómicas y Geofísicas - Universidad Nacional de La Plata Paseo del Bosque s/n. La Plata, Argentina email: [email protected]
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Abstract

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We present the Catalogue of High REsolution Spectra of Obscured Sources (CHRESOS) from the XMM-Newton Science Archive. It comprises soft X-ray emission-lines from C to Si and the Fe 3C and Fe 3G L-shell transitions. Here, we concentrate on the oxygen emission-lines O VII(f) and O VIII Lyα to shed light onto the physical processes with which their formation can be related to: active galactic nucleus vs. star-forming regions. We are analysing the relationships between the oxygen lines and the luminosities of: [OIII]λ5007, [OIV]25.89μm, MIR-12μm, FIR-60μm, FIR-100μm, and hard X-rays continuum bands.

Keywords

line: formationplasmasgalaxies: activegalaxies: Seyfert
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S359: Galaxy Evolution and Feedback across Different Environments , March 2019 , pp. 360 - 361
Copyright
© The Author(s), 2021. Published by Cambridge University Press on behalf of International Astronomical Union

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