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OB Associations and their origins
DOI: 10.1016/j.newar.2020.101549 Bibcode: 2020NewAR..9001549W

Wright, Nicholas J.

OB associations are unbound groups of young stars made prominent by their bright OB members, and have long been thought to be the expanded remnants of dense star clusters. They have been important in astrophysics for over a century thanks to their luminous massive stars, though their low-mass members have not been well studied until the last coupl…

2020 New Astronomy Reviews
Gaia 41
SS433: A massive X-ray binary in an advanced evolutionary stage
DOI: 10.1016/j.newar.2020.101542 Bibcode: 2020NewAR..8901542C

Cherepashchuk, Anatol; Postnov, Konstantin; Molkov, Sergey +2 more

INTEGRAL IBIS/ISGRI 18-60 keV observations of SS433 performed in 2003-2011 enabled for the first time the hard X-ray phase-resolved orbital and precessional light curves and spectra to be constructed. The spectra can be fitted by a power-law with photon index ≃ 3.8 and remain almost constant while the X-ray flux varies by a factor of a few. This s…

2020 New Astronomy Reviews
INTEGRAL 17
INTEGRAL View on cataclysmic variables and symbiotic binaries
DOI: 10.1016/j.newar.2020.101547 Bibcode: 2020NewAR..9101547L

Doroshenko, Victor; de Martino, Domitilla; Falanga, Maurizio +5 more

Accreting white dwarfs (WDs) constitute a significant fraction of the hard X-ray sources detected by the INTEGRAL observatory. Most of them are magnetic Cataclysmic Variables (CVs) of the intermediate polar (IP) and polar types, but the contribution of the Nova-likes systems and the systems with optically thin boundary layers, Dwarf Novae (DNs) an…

2020 New Astronomy Reviews
INTEGRAL 14
The Galactic LMXB Population and the Galactic Centre Region
DOI: 10.1016/j.newar.2020.101536 Bibcode: 2020NewAR..8801536S

Krivonos, R.; Sazonov, S.; Wilms, J. +21 more

Seventeen years of hard X-ray observations with the instruments of the INTEGRAL observatory, with a focus on the Milky Way and in particular on the Galactic Centre region, have provided a unique database for exploration of the Galactic population of low-mass X-ray binaries (LMXBs). Our understanding of the diverse energetic phenomena associated wi…

2020 New Astronomy Reviews
INTEGRAL 9
INTEGRAL results on the electron-positron annihilation radiation and X-ray & Gamma-ray diffuse emission of the Milky Way
DOI: 10.1016/j.newar.2020.101548 Bibcode: 2020NewAR..9001548C

Churazov, Eugene; Sunyaev, Rashid; Knödlseder, Jürgen +8 more

This review summarizes INTEGRAL results on two topics: the electron-positron annihilation line and X-ray & Gamma-ray diffuse emission of the Milky Way.

The electron-positron annihilation line at 511 keV is the most prominent spectral feature in the gamma-ray spectrum of the Milky Way. From the observational perspective, INTEGRAL has alrea…

2020 New Astronomy Reviews
INTEGRAL 9
The INTEGRAL view of the pulsating hard X-ray sky: from accreting and transitional millisecond pulsars to rotation-powered pulsars and magnetars
DOI: 10.1016/j.newar.2020.101544 Bibcode: 2020NewAR..9101544P

Tiengo, A.; Götz, D.; Mereghetti, S. +30 more

In the last 25 years a new generation of X-ray satellites imparted a significant leap forward in our knowledge of X-ray pulsars. The discovery of accreting and transitional millisecond pulsars proved that disk accretion can spin up a neutron star to a very high rotation speed. The detection of MeV-GeV pulsed emission from a few hundreds of rotatio…

2020 New Astronomy Reviews
INTEGRAL 7
INTEGRAL view of AGN
DOI: 10.1016/j.newar.2020.101545 Bibcode: 2020NewAR..9001545M

Pian, Elena; Sazonov, Sergey; Bassani, Loredana +5 more

AGN are among the most energetic phenomena in the Universe and in the last two decades INTEGRAL's contribution in their study has had a significant impact. Thanks to the INTEGRAL extragalactic sky surveys, all classes of soft X-ray detected (in the 2-10 keV band) AGN have been observed at higher energies as well. Up to now, around 450 AGN have bee…

2020 New Astronomy Reviews
INTEGRAL 5