Search Publications

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
X-Ray Spectroscopy in the Microcalorimeter Era. II. A New Diagnostic on Column Density from the Case A to B Transition in H- and He-like Iron
DOI: 10.3847/1538-4357/abaaac Bibcode: 2020ApJ...901...69C

Ferland, G. J.; Su, Y.; Chakraborty, P. +2 more

The Soft X-ray Spectrometer on board Hitomi, with the unprecedented resolving power of R ∼ 1250, allowed the detection of members of the Fe XXV Kα complex emission spectra from the center of the Perseus Cluster. In this paper, we introduce a novel method of measuring the column density using the optically thin (Case A) to optically thick (Case B) …

2020 The Astrophysical Journal
Hitomi 15
Hubble Space Telescope Search for Activity in High-perihelion Objects
DOI: 10.3847/1538-3881/ab7faf Bibcode: 2020AJ....159..209L

Mutchler, Max; Jewitt, David; Agarwal, Jessica +2 more

Solar system objects with perihelia beyond the orbit of Jupiter (q > 5 au) are too cold for water ice to generate an appreciable coma via sublimation. Despite this, numerous high-perihelion objects (HPOs) including many comets and recently escaped Kuiper Belt objects (Centaurs) are observed to be active out at least to the orbit of Saturn (q ∼ …

2020 The Astronomical Journal
eHST 15
Kinematical investigation of possible fast collimated outflows in twelve planetary nebulae
DOI: 10.1093/mnras/stz3326 Bibcode: 2020MNRAS.492.1957R

Chu, Y. -H.; Guerrero, M. A.; Toalá, J. A. +3 more

A significant fraction of planetary nebulae (PNe) exhibit collimated outflows, distinct narrow kinematical components with notable velocity shifts with respect to the main nebular shells typically associated with low-ionization compact knots and linear or precessing jet-like features. We present here a spatio-kinematical investigation of a sample …

2020 Monthly Notices of the Royal Astronomical Society
eHST 15
Constraining the Mass of the Emerging Galaxy Cluster SpARCS1049+56 at z = 1.71 with Infrared Weak Lensing
DOI: 10.3847/1538-4357/ab7bdb Bibcode: 2020ApJ...893...10F

Muzzin, Adam; Perlmutter, Saul; Wilson, Gillian +4 more

In the hierarchical structure formation model of the universe, galaxy clusters are assembled through a series of mergers. Accordingly, it is expected that galaxy clusters in the early universe are actively forming and dynamically young. Located at a high redshift of z = 1.71, SpARCS1049+56 offers a unique look into the galaxy cluster formation pro…

2020 The Astrophysical Journal
eHST 15