The changing milliarcsecond radio morphology of the gamma-ray binary LS 5039

2008/01/25 by M. Ribo, M. Ribó, J. M. Paredes +5 · 3 citations
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysical Phenomena and Observations #Astrophysics and Cosmic Phenomena #astro-ph

paper · pdf · doi:10.1051/0004-6361:20078390

published as Astron.Astrophys. 481 (2008) 17-20 · To be published in A&A main journal. 5 pages, 1 figure. A reference has been corrected

openalex publication_date 2008/01/25 · arxiv created 2008/02/01 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/01

Abstract

Context.LS 5039 is one of the few TeV emitting X-ray binaries detected so far. The powering source of its multiwavelength emission can be accretion in a microquasar scenario or wind interaction in a young nonaccreting pulsar scenario.

Cited by

• LONG-TERM STABILITY OF NONTHERMAL X-RAY MODULATION IN THE GAMMA-RAY BINARY LS 5039
• DISCOVERY OF EXTENDED AND VARIABLE RADIO STRUCTURE FROM THE GAMMA-RAY BINARY SYSTEM PSR B1259–63/LS 2883
• Studying the properties of the radio emitter in LS 5039

Related

• Exploring the powering source of the TeV X-ray binary LS 5039
• The astrometric/morphological variability and the birth place of LS 5039
• The TeV emitter structure in LS 5039
• The gamma-ray binaries LS 5039, LS I +61 303 and PSR B1259-63
• LONG-TERM STABILITY OF NONTHERMAL X-RAY MODULATION IN THE GAMMA-RAY BINARY LS 5039