Rapid variability of the compact radio sources in Arp220 Evidence for a population of microblazars?
Artikel i vetenskaplig tidskrift, 2012

Context. The two nuclei of the starburst galaxy Arp220 contain multiple compact radio sources previously identified as radio supernovae or supernova remnants. Aims. In order to search for an embedded radio AGN, or other possible exotic objects, we have carried out a programme of VLBI monitoring at 6 cm over three epochs each separated by four months. Methods. Combining the new data with existing data at 6 cm and 18 cm (spanning 4 and 12 years respectively) we are able to characterise source flux density variability on a range of timescales. Additionally we analyse the variability of sources in shape and position. Results. We detect rapid (<4 months) variability in three sources (W7, W26, and W29). These sources show possible superluminal motion (>4c) of jet-like features near rapidly varying almost stationary components. These enigmatic sources might be associated with an AGN or a highly beamed microquasar (i.e. microblazar). Other hypotheses include that the apparent variability is intrinsic and is produced by neutron star powered central components within a supernova remnant, by a sequence of several supernovae within super star clusters, or is extrinsic and is produced by Galactic interstellar scintillation of very compact non-varying objects. Conclusions. A microquasar/microblazar origin seems to be the best explanation for the nature of the variable sources in Arp220.

radio continuum: stars

light-curves

galaxies: starburst

supernova-remnants

black-hole

galaxies: nuclei

starburst

X-rays:

galaxy

galaxies: individual: Arp220

arp-220

vlbi

nucleus

candidates

m82

Författare

Fabien Batejat

Chalmers, Rymd- och geovetenskap, Onsala rymdobservatorium

John Conway

Chalmers, Rymd- och geovetenskap, Onsala rymdobservatorium

Anthony Rushton

Chalmers, Rymd- och geovetenskap, Onsala rymdobservatorium

R. Parra

P. J. Diamond

C. J. Lonsdale

Astronomy and Astrophysics

0004-6361 (ISSN) 1432-0746 (eISSN)

Vol. 542 L24

Ämneskategorier

Astronomi, astrofysik och kosmologi

DOI

10.1051/0004-6361/201219235