The Chandra High Resolution Spectra of Mkn 421

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dc.creatorNicastro, F.
dc.creatorFruscione, A.
dc.creatorElvis, M.
dc.creatorSiemiginowska, A.
dc.creatorFiore, F.
dc.creatorBianchi, S.
dc.date2001-02-26
dc.date.accessioned2026-07-07T01:57:50Z
dc.date.available2026-07-07T01:57:50Z
dc.descriptionMkn 421 was observed by Chandra twice, on November 5, 1999 as part of the Chandra calibration program, with the ACIS-HETG configuration, and on May 29, 2000 following our Target Of Opportunity request aimed to catch the source in an ultra-high state, with both the ACIS-HETG and the HRC-LETG configurations. In this contribution we present and compare the two Chandra-MEG observations of Mkn 421, which lasted 26 and 19.6 ks respectively.
dc.description6 pages, 2 figures. To appear in the proceedings of the "X-Ray Astronomy 2000" conference (Sept. 2000, Palermo, Italy), PASP Conference Series, ed. R. Giacconi, L. Stella and S. Serio
dc.identifierhttps://arxiv.org/abs/astro-ph/0102455
dc.identifierhttp://arxiv.org/abs/astro-ph/0102455
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2540
dc.subjectAstrophysics
dc.titleThe Chandra High Resolution Spectra of Mkn 421
dc.typetext

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