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Search: (WFRF:(Hada K.)) srt2:(2015-2019) > (2016) > The origin of Fast ...

The origin of Fast Radio Bursts, still an open question

Marcote, B. (author)
Joint Institute for VLBI in Europe (JIVE)
Giroletti, M. (author)
Istituto di Radioastronomia
Garrett, M. A. (author)
Netherlands Institute for Radio Astronomy (ASTRON)
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Paragi, Z. (author)
Joint Institute for VLBI in Europe (JIVE)
Yang, Jian, 1960 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Hada, K. (author)
National Astronomical Observatory of Japan
Cheung, C.C. (author)
Naval Research Laboratory
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 (creator_code:org_t)
2016
2016
English.
In: Proceedings of the 12th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics IX, SEA 2016.
  • Conference paper (peer-reviewed)
Abstract Subject headings
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  • FRB 150418 is the first Fast Radio Burst (FRB) with a proposed counterpart. Keane et al. (2016) claimed that the galaxy WISE J0716-19 is the host of this event. Such association would provide extremely important clues about the possible extragalactic origin of the FRBs. It is still a mystery what kind of events produces the FRBs. We observed the proposed host galaxy with the European VLBI Network (EVN) during four epochs at 5 GHz, revealing a compact and persistent radio source located in the center of the galaxy. These data, together with contemporaneous observations, strongly support the presence of an active galactic nuclei (AGN) in the galaxy with variability on short timescales due to refractive scintillation. Therefore, WISE J0716-19 would not be related with FRB 150418.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

Pulsars
Astrophysics
Radio bursts
Diethylaminoethyldextran

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Marcote, B.
Giroletti, M.
Garrett, M. A.
Paragi, Z.
Yang, Jian, 1960
Hada, K.
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Cheung, C.C.
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NATURAL SCIENCES
NATURAL SCIENCES
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and Astronomy Astrop ...
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Chalmers University of Technology

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