Redshifted Fe K alpha line from the unusual gamma-ray source PMN J1603-4904

Mueller C, Krauss F, Dauser T, Kreikenbohm A, Beuchert T, Kadler M, Ojha R, Wilms J, Boeck M, Carpenter B, Dutka M, Markowitz A, Mcconville W, Pottschmidt K, Stawarz L, Taylor GB (2015)

Publication Status: Published

Publication Type: Journal article, other

Publication year: 2015

Journal

Astronomy & Astrophysics EDP Sciences

Publisher: EDP Sciences

Book Volume: 574

DOI: 10.1051/0004-636/201425442

Abstract

Conclusions. The detection of a redshiftecl X-ray emission line further challenges the original BL Lac classification of PMN J1603-4904. This result suggests that the source is observed at a larger angle to the line of sight than expected for blazars. and thus the source would add to the elusive class of gamma-ray loud misaligned jet objects, possibly a gamma-ray bright young radio galaxy.

Authors with CRIS profile

Thomas Dauser Dr.Karl-Remeis-Sternwarte Bamberg, Astronomisches Institut Jörn Wilms Professur für Astronomie und Astrophysik Alex Markowitz Dr.Karl-Remeis-Sternwarte Bamberg, Astronomisches Institut

Involved external institutions

University of New Mexico (UNM) / Universidad de Nuevo México

United States (USA) (US) Japan Aerospace eXploration Agency (JAXA)

Japan (JP) University of Maryland, Baltimore County (UMBC)

United States (USA) (US) University of Maryland

United States (USA) (US) Julius-Maximilians-Universität Würzburg

Germany (DE)

How to cite

APA:

Mueller, C., Krauss, F., Dauser, T., Kreikenbohm, A., Beuchert, T., Kadler, M.,... Taylor, G.B. (2015). Redshifted Fe K alpha line from the unusual gamma-ray source PMN J1603-4904. Astronomy & Astrophysics, 574. https://doi.org/10.1051/0004-636/201425442

MLA:

Mueller, C., et al. "Redshifted Fe K alpha line from the unusual gamma-ray source PMN J1603-4904." Astronomy & Astrophysics 574 (2015).

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