Search Publications

Ram pressure stripping in high-density environments
DOI: 10.1007/s00159-022-00140-3 Bibcode: 2022A&ARv..30....3B

Fossati, Matteo; Sun, Ming; Boselli, Alessandro

Galaxies living in rich environments are suffering different perturbations able to drastically affect their evolution. Among these, ram pressure stripping, i.e. the pressure exerted by the hot and dense intracluster medium (ICM) on galaxies moving at high velocity within the cluster gravitational potential well, is a key process able to remove the…

2022 Astronomy and Astrophysics Review
XMM-Newton eHST 204
Supernova remnants: the X-ray perspective
DOI: 10.1007/s00159-011-0049-1 Bibcode: 2012A&ARv..20...49V

Vink, Jacco

Supernova remnants are beautiful astronomical objects that are also of high scientific interest, because they provide insights into supernova explosion mechanisms, and because they are the likely sources of Galactic cosmic rays. X-ray observations are an important means to study these objects. And in particular the advances made in X-ray imaging s…

2012 Astronomy and Astrophysics Review
XMM-Newton 400
Non-thermal emission processes in massive binaries
DOI: 10.1007/s00159-007-0005-2 Bibcode: 2007A&ARv..14..171D

De Becker, Michaël

In this paper, I present a general discussion of several astrophysical processes likely to play a role in the production of non-thermal emission in massive stars, with emphasis on massive binaries. Even though the discussion will start in the radio domain where the non-thermal emission was first detected, the census of physical processes involved …

2007 Astronomy and Astrophysics Review
XMM-Newton 118
X-ray astronomy of stellar coronae
DOI: 10.1007/s00159-004-0023-2 Bibcode: 2004A&ARv..12...71G

Güdel, Manuel

X-ray emission from stars in the cool half of the Hertzsprung-Russell diagram is generally attributed to the presence of a magnetic corona that contains plasma at temperatures exceeding 1 million K. Coronae are ubiquitous among these stars, yet many fundamental mechanisms operating in their magnetic fields still elude an interpretation through a d…

2004 Astronomy and Astrophysics Review
XMM-Newton 406