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The tidal stream generated by the globular cluster NGC 3201
DOI: 10.1093/mnras/stab1024 Bibcode: 2021MNRAS.504.2727P

Miralda-Escudé, Jordi; Palau, Carles G.

We detect a tidal stream generated by the globular cluster NGC 3201 extending over ~140 deg on the sky, using the Gaia DR2 data, with the maximum-likelihood method we presented previously to study the M68 tidal stream. Most of the detected stream is the trailing one, which stretches in the southern Galactic hemisphere and passes within a close dis…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 17
TESS Observations of Be Stars: General Characteristics and the Impulsive Magnetic Rotator Model
DOI: 10.3847/1538-4357/ac1a77 Bibcode: 2021ApJ...921....5B

Balona, Luis A.; Ozuyar, Dogus

Evidence of rotational light modulation in 30%-40% of normal B stars is presented, suggesting the presence of starspots and photospheric activity. On this basis, we propose that mass loss in Be stars is a result of magnetic reconnection coupled with rapid but not necessarily near-critical rotation. The ejected matter is trapped at two diametricall…

2021 The Astrophysical Journal
Gaia 17
Analytical Framework for Space Debris Collision Avoidance Maneuver Design
DOI: 10.2514/1.G005398 Bibcode: 2021JGCD...44..469G

Di Lizia, Pierluigi; Colombo, Camilla; Gonzalo, Juan Luis

An analytical formulation for collision avoidance maneuvers involving a spacecraft and a space debris is presented, including solutions for the maximum deviation and minimum collision probability cases. Gauss' planetary equations and relative motion equations are used to map maneuvers at a given time to displacements at the predicted close approac…

2021 Journal of Guidance Control Dynamics
PROBA-2 XMM-Newton 17
ALMA and IRIS Observations of the Solar Chromosphere. II. Structure and Dynamics of Chromospheric Plages
DOI: 10.3847/1538-4357/abc9b0 Bibcode: 2021ApJ...906...83C

Martínez-Sykora, Juan; De Pontieu, Bart; Chintzoglou, Georgios +7 more

We propose and employ a novel empirical method for determining chromospheric plage regions, which seems to better isolate a plage from its surrounding regions than other methods commonly used. We caution that isolating a plage from its immediate surroundings must be done with care in order to successfully mitigate statistical biases that, for inst…

2021 The Astrophysical Journal
IRIS 17
Lessons learned from SPHERE for the astrometric strategy of the next generation of exoplanet imaging instruments
DOI: 10.1117/1.JATIS.7.3.035004 Bibcode: 2021JATIS...7c5004M

Henning, Thomas; Boccaletti, Anthony; Wahhaj, Zahed +14 more

Measuring the orbits of directly imaged exoplanets requires precise astrometry at the milliarcsec level over long periods of time due to their wide separation to the stars (≳10 au) and long orbital period (≳20 yr). To reach this challenging goal, a specific strategy was implemented for the instrument Spectro-Polarimetric High-contrast Exoplanet Re…

2021 Journal of Astronomical Telescopes, Instruments, and Systems
Gaia 17
Radio pulsations from the γ-ray millisecond pulsar PSR J2039-5617
DOI: 10.1093/mnras/staa3463 Bibcode: 2021MNRAS.502..935C

Belfiore, A.; Venter, C.; Possenti, A. +9 more

The predicted nature of the candidate redback pulsar 3FGL J2039.6-5618 was recently confirmed by the discovery of γ-ray millisecond pulsations (Clark et al., hereafter Paper I), which identify this γ-ray source as PSR J2039-5617. We observed this object with the Parkes radio telescope in 2016 and 2019. We detect radio pulsations at 1.4 and 3.1 GHz…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 17
Compton-Thick AGN in the NuSTAR ERA VII. A joint NuSTAR, Chandra, and XMM-Newton Analysis of Two Nearby, Heavily Obscured Sources
DOI: 10.3847/1538-4357/ac1fee Bibcode: 2021ApJ...922..159T

Vignali, C.; Gilli, R.; Ajello, M. +11 more

We present the joint Chandra, XMM-Newton, and NuSTAR analysis of two nearby Seyfert galaxies, NGC 3081 and ESO 565-G019. These are the only two having Chandra data in a larger sample of 10 low-redshift (z ≤ 0.05), candidates Compton-thick (CT) Active Galactic Nuclei selected in the 15-150 keV band with Swift-BAT that were still lacking NuSTAR data…

2021 The Astrophysical Journal
XMM-Newton 17
A search for satellite galaxies of nearby star-forming galaxies with resolved stars in LBT-SONG
DOI: 10.1093/mnras/stab2447 Bibcode: 2021MNRAS.507.4764G

Kochanek, Christopher S.; Sand, David J.; Peter, Annika H. G. +2 more

We present results from a resolved stellar population search for dwarf satellite galaxies of six nearby (D < 5 Mpc), sub-Milky Way mass hosts using deep (m ~ 27 mag) optical imaging from the Large Binocular Telescope. We perform image simulations to quantify our detection efficiency for dwarfs over a large range in luminosity and size, and deve…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 17
Beyond Simple AGN Unification with Chandra-observed 3CRR Sources at 0.5 < z < 1
DOI: 10.3847/1538-4357/abf3c0 Bibcode: 2021ApJ...913..134K

Azadi, Mojegan; Wilkes, Belinda J.; McDowell, Jonathan C. +14 more

Low-frequency radio selection finds radio-bright galaxies regardless of the amount of obscuration by gas and dust. We report Chandra observations of a complete 178 MHz-selected, and so orientation-unbiased, sample of 44 0.5 < z < 1 3CRR sources. The sample is comprised of quasars and narrow-line radio galaxies (NLRGs) with similar radio lumi…

2021 The Astrophysical Journal
Herschel 17
Exploring the Stellar Rotation of Early-type Stars in the LAMOST Medium-resolution Survey. I. Catalog
DOI: 10.3847/1538-4365/ac1acf Bibcode: 2021ApJS..257...22S

Deng, Licai; de Grijs, Richard; Liu, Chao +3 more

We derive stellar parameters and abundances ("stellar labels") of 40,034 late-B and A-type main-sequence stars extracted from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope Medium Resolution Survey (LAMOST-MRS). The primary selection of our early-type sample was obtained from LAMOST Data Release 7 based on spectral-line indices. We …

2021 The Astrophysical Journal Supplement Series
Gaia 17