2004A&A...424..747P


C.D.S. - SIMBAD4 rel 1.7 - 2021.02.27CET00:24:32

2004A&A...424..747P - Astronomy and Astrophysics, volume 424, 747-760 (2004/9-4)

Superbubbles and energetic particles in the Galaxy. I. Collective effects of particle acceleration.

PARIZOT E., MARCOWITH A., VAN DER SWALUW E., BYKOV A.M. and TATISCHEFF V.

Abstract (from CDS):

Observations indicate that most massive stars in the Galaxy appear in groups, called OB associations, where their strong wind activity generates large structures known as superbubbles, inside which the subsequent supernovae (SNe) explode, with a tight space and time correlation. We investigate four main questions: 1) does the clustering of massive stars and SN explosions influence the particle acceleration process usually associated with SNe, and induce collective effects which would not manifest around isolated supernova remnants?; 2) does it make a difference for the general phenomenology of Galactic Cosmic Rays (GCRs), notably for their energy spectrum and composition?; 3) Can this help alleviate some of the problems encountered within the standard GCR source model?; and 4) Is the link between superbubbles and energetic particles supported by observational data, and can it be further tested and constrained? We argue for a positive answer to all these questions. Theoretical, phenomenological and observational aspects are treated in separate papers. Here, we discuss the interaction of massive stellar winds and SN shocks inside superbubbles and indicate how this leads to specific acceleration effects. We also show that due to the high SN explosion rate and low diffusion coefficient, low-energy particles experience repeated shock acceleration inside superbubbles.

Abstract Copyright:

Journal keyword(s): ISM: cosmic rays - acceleration of particles - ISM: supernovae remnants - shock waves - ISM: bubbles

Simbad objects: 2

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Number of rows : 2

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
#notes
1 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 15196 1
2 LHA 120-N 51D HII 05 25 17.3 -67 22 47           ~ 108 0

    Equat.    Gal    SGal    Ecl

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2021.02.27-00:24:32

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