Filming the evolution of symbiotic novae with VLBI: The 2021 explosion of RS Oph
Paper i proceeding, 2023

Fifteen years after its previous outburst, the symbiotic recurrent nova RS Oph exploded again on 2021 Aug 8th, its first outburst during the Fermi era. In symbiotic novae, the material ejected from the surface of the white dwarf (WD) after the thermonuclear runaway drives a strong shock through the dense circumstellar gas produced by the red giant (RG) wind. This nova is a perfect real-Time laboratory for studying physical processes as diverse as accretion, thermonuclear explosions, shock dynamics and particle acceleration; in many ways it is like a supernova remnant on fast forward. The experience of its previous outburst and that of 2010 for V407 (the symbiotic nova that has been extensively observed during the Fermi era), indicates that a large sensitivity and a broad range of baseline lengths are necessary to follow its evolution over a period of several weeks. This would provide unique constraints on major outstanding problems, including the emission mechanisms, the physical processes at work, the presence and location of shock acceleration, the geometry of the system, and the density of the RG wind. We present preliminary results from the EVN+e-MERLIN observations carried out on weeks/months time scales after the August explosion.

Författare

M. Giroletti

Istituto di Radioastronomia

U. Munari

Istituto nazionale di astrofisica (INAF)

B. Marcote

JOINT INSTITUTE FOR V.L.B.I. IN EUROPE (J.I.V.E.)

Tim O'Brien

University of Manchester

P. Veres

Center for Space Plasma and Aeronomic Research

Jun Yang

Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium

D. R.A. Williams

University of Manchester

P. A. Woudt

University of Cape Town

Proceedings of Science

18248039 (eISSN)

Vol. 428 038

15th European VLBI Network Mini-Symposium and Users' Meeting, EVN 2022
Cork, Ireland,

Ämneskategorier

Astronomi, astrofysik och kosmologi

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Senast uppdaterat

2024-11-27