A characterization of the NGC 4051 soft X-ray spectrum as observed by XMM-Newton

Astronomy and Astrophysics

Volumn 515, Issue 6, 2010, Pages

  Nucita, A A ^a   Guainazzi, M ^a   Longinotti, A L ^b   Santos Lleo, M ^a   Maruccia, Y ^c   Bianchi, S ^d  

^a EUROPEAN SPACE AGENCY   (Spain)

^b MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^c UNIVERSITY OF SALENTO   (Italy)

^d ROMA TRE UNIVERSITY   (Italy)

Author keywords

Galaxies: individual: NGC 4051; Galaxies: Seyfert; Techniques: spectroscopic

Indexed keywords

CARRIER CONCENTRATION; ELECTROMAGNETIC WAVE EMISSION; ELECTRON DENSITY MEASUREMENT; GALAXIES; IONIZATION OF GASES; IRON COMPOUNDS; METAL IONS; NEON; PARTICLE DETECTORS; PHOTOIONIZATION; PHYSICAL PROPERTIES; RADIOACTIVITY LOGGING; SPECTROSCOPIC ANALYSIS; X RAY ANALYSIS; X RAY SPECTROGRAPHS; X RAYS;

ATOMIC TRANSITION; CENTRAL ENGINES; COLUMN DENSITY; DIAGNOSTIC TOOLS; ELECTRON DENSITIES; EMISSION LINES; GALAXIES: SEYFERT; GALAXIES:INDIVIDUAL:NGC 4051; HIGH-RESOLUTION SPECTROSCOPY; HYDROGEN COLUMN DENSITY; IONIZATION PARAMETER; IRON IONS; L SHELL; LOW FLUX; PHASE GAS; PHOTOIONIZED PLASMAS; SEYFERTS; SINGLE PHOTO IONIZATION; SOFT X-RAY; SPECTRAL FEATURE; SYNTHETIC MODELS; X-RAY EMITTING; XMM-NEWTON;

ATOMIC SPECTROSCOPY;

EID: 77953249918     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913673     Document Type: Article

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