The BeppoSAX X-ray view of reflection-dominated Seyfert Galaxies

F.Fiore (3) ((1) Astrophysics Division; G.Matt (2); I); I; (3) Osservatorio Astronomico di Roma; M.Guainazzi (1); Monteporzio Catone; NL; (2) Universita' Roma 3; Noordwijk; SSD of ESA

REVIEW

The BeppoSAX X-ray view of reflection-dominated Seyfert Galaxies

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv astro-ph/9902322 v1 pith:T2L3JF7A submitted 1999-02-23 astro-ph

M.Guainazzi (1) , G.Matt (2) , F.Fiore (3) ((1) Astrophysics Division , SSD of ESA , Noordwijk , NL; (2) Universita' Roma 3 , I; (3) Osservatorio Astronomico di Roma , Monteporzio Catone

show 1 more author

This is my paper · ORCID

classification astro-ph

keywords seyfertx-raybepposaxgalaxiesreflection-dominatedactivitycircinuscomponent

verification ladder T0 review T1 audit T2 compute T3 formal

0 comments

read the original abstract

We present new results from BeppoSAX observations of reflection-dominated Seyfert galaxies, and namely: 1) the Compton-thick Seyfert 2s NGC1068 and Circinus Galaxy; 2) the Seyfert 1 NGC4051, whose nucleus was observed on May 1998 to have switched off, leaving only a residual reflection component as an echo of its past activity. Our main focus in this paper is on the soft X-ray continuum properties and on the X-ray line spectroscopy.

Discussion (0). Continue with ORCID to comment.

Pith tools