Search Publications

Fast radio bursts at the dawn of the 2020s
DOI: 10.1007/s00159-022-00139-w Bibcode: 2022A&ARv..30....2P

Lorimer, D. R.; Hessels, J. W. T.; Petroff, E.

Since the discovery of the first fast radio burst (FRB) in 2007, and their confirmation as an abundant extragalactic population in 2013, the study of these sources has expanded at an incredible rate. In our 2019 review on the subject, we presented a growing, but still mysterious, population of FRBs—60 unique sources, 2 repeating FRBs, and only 1 i…

2022 Astronomy and Astrophysics Review
INTEGRAL 263
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
The evolution of CNO elements in galaxies
DOI: 10.1007/s00159-022-00144-z Bibcode: 2022A&ARv..30....7R

Romano, Donatella

After hydrogen and helium, oxygen, carbon, and nitrogen—hereinafter, the CNO elements—are the most abundant species in the universe. They are observed in all kinds of astrophysical environments, from the smallest to the largest scales, and are at the basis of all known forms of life, hence, the constituents of any biomarker. As such, their study p…

2022 Astronomy and Astrophysics Review
Gaia 34
Low-energy cosmic rays: regulators of the dense interstellar medium
DOI: 10.1007/s00159-022-00141-2 Bibcode: 2022A&ARv..30....4G

Gabici, Stefano

Low-energy cosmic rays (up to the GeV energy domain) play a crucial role in the physics and chemistry of the densest phase of the interstellar medium. Unlike interstellar ionising radiation, they can penetrate large column densities of gas, and reach molecular cloud cores. By maintaining there a small but not negligible gas ionisation fraction, th…

2022 Astronomy and Astrophysics Review
INTEGRAL 31