Search Publications

Kinematics of the Magellanic Stream and Implications for Its Ionization
DOI: 10.3847/1538-4357/ab92a3 Bibcode: 2020ApJ...897...23F

Richter, Philipp; Bland-Hawthorn, Joss; Fox, Andrew J. +3 more

The Magellanic Stream and the Leading Arm form a massive, filamentary system of gas clouds surrounding the Large and Small Magellanic Clouds. Here we present a new component-level analysis of their ultraviolet (UV) kinematic properties using a sample of 31 sightlines through the Magellanic System observed with the Hubble Space Telescope/Cosmic Ori…

2020 The Astrophysical Journal
eHST 15
5D memberships and fundamental properties of the old open cluster NGC 6791 based on Gaia-DR2
DOI: 10.1007/s10509-020-3738-2 Bibcode: 2020Ap&SS.365...24G

Gao, Xinhua

This paper investigates reliable memberships and fundamental astrophysical properties of the old (∼8 Gyr) open cluster NGC 6791 using the astrometric and photometric data of the Gaia data release 2 (Gaia-DR2). We identify 2536 likely cluster membe…

2020 Astrophysics and Space Science
Gaia 15
The WAGGS project-III. Discrepant mass-to-light ratios of Galactic globular clusters at high metallicity
DOI: 10.1093/mnras/staa091 Bibcode: 2020MNRAS.492.3859D

Martocchia, S.; Da Costa, G. S.; Usher, C. +10 more

Observed mass-to-light ratios (M/L) of metal-rich globular clusters (GCs) disagree with theoretical predictions. This discrepancy is of fundamental importance since stellar population models provide the stellar masses that underpin most of extragalactic astronomy, near and far. We have derived radial velocities for 1622 stars located in the centre…

2020 Monthly Notices of the Royal Astronomical Society
Gaia eHST 15
High-resolution X-ray spectroscopy of the stellar wind in Vela X-1 during a flare
DOI: 10.1051/0004-6361/202037807 Bibcode: 2020A&A...641A.144L

Bianchi, S.; Guainazzi, M.; Grinberg, V. +8 more

Context. We present a ~130 ks observation of the prototypical wind-accreting, high-mass X-ray binary Vela X-1 collected with XMM-Newton at orbital phases between 0.12 and 0.28. A strong flare took place during the observation that allows us to investigate the reaction of the clumpy stellar wind to the increased X-ray irradiation.
Aims: To exa…

2020 Astronomy and Astrophysics
Gaia XMM-Newton 15
Reflection component in the Bright Atoll Source GX 9+9
DOI: 10.1051/0004-6361/202037491 Bibcode: 2020A&A...635A.209I

Sanna, A.; Di Salvo, T.; Burderi, L. +5 more

Context. GX 9+9 (4U 1728-16) is a low mass X-ray binary source harboring a neutron star. Although it belongs to the subclass of the bright Atoll sources together with GX 9+1, GX 3+1, and GX 13+1, its broadband spectrum is poorly studied and apparently does not show reflection features in the spectrum.
Aims: To constrain the continuum well and…

2020 Astronomy and Astrophysics
XMM-Newton 15
Outstanding questions in magnetospheric plasma physics: The pollenzo view
DOI: 10.1016/j.jastp.2020.105377 Bibcode: 2020JASTP.20805377B

Stepanova, Marina; Hesse, Michael; Delzanno, Gian Luca +6 more

Based on discussions held at a workshop in Bra-Pollenzo, Italy, this paper elaborates upon 19 outstanding questions of plasma physics in the Earth's magnetosphere. The questions are grouped according to (a) driving processes, (b) radiation belt and ring current issues, (c) auroral physics, (d) internal plasma processes, and (e) magnetosphere-ionos…

2020 Journal of Atmospheric and Solar-Terrestrial Physics
Cluster 15
Chromosome maps of young LMC clusters: an additional case of coeval multiple populations
DOI: 10.1093/mnras/staa644 Bibcode: 2020MNRAS.493.6060S

Martocchia, S.; Dalessandro, E.; Salaris, M. +9 more

Recent studies have revealed that the multiple populations (MPs) phenomenon does not occur only in ancient and massive Galactic globular clusters (GCs), but it is also observed in external galaxies, where GCs sample a wide age range with respect to the Milky Way. However, for a long time, it was unclear whether we were looking at the same phenomen…

2020 Monthly Notices of the Royal Astronomical Society
Gaia eHST 15
X-ray absorption in INTEGRAL active galactic nuclei. Host galaxy inclination
DOI: 10.1051/0004-6361/202038014 Bibcode: 2020A&A...639A...5M

Ubertini, P.; Malizia, A.; Bassani, L. +2 more

In this work the INTEGRAL hard X-ray selected sample of active galactic nuclei (AGN) has been used to investigate the possible contribution of absorbing material distributed within the host galaxies to the total amount of NH measured in the X-ray band. We collected all the available axial ratio measurements of the galaxies hosting our A…

2020 Astronomy and Astrophysics
INTEGRAL 15
An Accreting, Anomalously Low-mass Black Hole at the Center of Low-mass Galaxy IC 750
DOI: 10.3847/1538-4357/ab9944 Bibcode: 2020ApJ...897..111Z

Gelfand, Joseph D.; Chen, Yan-Ping; Greenhill, Lincoln J. +5 more

We present a multiwavelength study of the active galactic nucleus in the nearby (D = 14.1 Mpc) low-mass galaxy IC 750, which has circumnuclear 22 GHz water maser emission. The masers trace a nearly edge-on, warped disk ∼0.2 pc in diameter, coincident with the compact nuclear X-ray source that lies at the base of the ∼kiloparsec-scale extended X-ra…

2020 The Astrophysical Journal
XMM-Newton eHST 15
A MeerKAT survey of nearby nova-like cataclysmic variables
DOI: 10.1093/mnras/staa1747 Bibcode: 2020MNRAS.496.2542H

Knigge, C.; Heywood, I.; Wijers, R. A. M. J. +17 more

We present the results of MeerKAT radio observations of 11 nearby nova-like cataclysmic variables (CVs). We have detected radio emission from IM Eri, RW Sex, V3885 Sgr, and V603 Aql. While RW Sex, V3885 Sgr, and V603 Aql had been previously detected, this is the first reported radio detection of IM Eri. Our observations have doubled the sample of …

2020 Monthly Notices of the Royal Astronomical Society
Gaia eHST 15