Deep X-ray view of the Class I YSO Elias 29 with XMM-Newton and NuSTAR

Autor:	Fabio Reale, Ettore Flaccomio, Giuseppina Micela, Beate Stelzer, Costanza Argiroffi, Ignazio Pillitteri, Salvatore Sciortino
Přispěvatelé:	ITA, DEU, Pillitteri, I., Sciortino, S., Reale, F., Micela, G., Argiroffi, C., Flaccomio, E., Stelzer, B.
Jazyk:	angličtina
Rok vydání:	2019
Předmět:	010504 meteorology & atmospheric sciences Young stellar object Astrophysics::High Energy Astrophysical Phenomena Population FOS: Physical sciences Astrophysics Astrophysics::Cosmology and Extragalactic Astrophysics 01 natural sciences law.invention Settore FIS/05 - Astronomia E Astrofisica law 0103 physical sciences Astrophysics::Solar and Stellar Astrophysics education 010303 astronomy & astrophysics Solar and Stellar Astrophysics (astro-ph.SR) Astrophysics::Galaxy Astrophysics 0105 earth and related environmental sciences Line (formation) Physics High Energy Astrophysical Phenomena (astro-ph.HE) education.field_of_study Star formation Astronomy and Astrophysics Corona Accretion (astrophysics) Astrophysics - Solar and Stellar Astrophysics Space and Planetary Science Astrophysics - High Energy Astrophysical Phenomena stars:activity–stars:coronae–stars:pre-mainsequence–stars:formation–stars:flare Equivalent width Flare
Popis:	[Abridged] We investigated the X-ray characteristics of the Class I YSO Elias 29 with joint XMM-Newton and NuSTAR observations of 300 ks and 450 ks, respectively. These are the first observations of a very young (7.11$ keV. 15 pages, 14 figures, accepted for publication on A&A
Databáze:	OpenAIRE
Externí odkaz:	https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b86f009231b62fc7dd365fc245ee8c3d http://hdl.handle.net/20.500.12386/30930 Zobrazit plný text záznamu