Search Publications

A Hard Look at Local, Optically Selected, Obscured Seyfert Galaxies
DOI: 10.3847/1538-4357/abb29f Bibcode: 2020ApJ...901..161K

Kaastra, J. S.; Stern, D.; Brandt, W. N. +11 more

We study the X-ray spectra of a sample of 19 obscured, optically selected Seyfert galaxies (Sy 1.8, 1.9, and 2) in the local universe (d ≤ 175 Mpc), drawn from the CfA Seyfert sample. Our analysis is driven by the high sensitivity of NuSTAR in the hard X-rays, coupled with soft X-ray spectra using XMM-Newton, Chandra, Suzaku, and Swift/XRT. We als…

2020 The Astrophysical Journal
Suzaku XMM-Newton 23
Binary Stars in Upper Scorpius
DOI: 10.3847/1538-3881/ab5525 Bibcode: 2020AJ....159...15T

Tokovinin, Andrei; Briceño, Cesar

To address the statistics of binary stars in the 8 Myr old Upper Scorpius (USco) star formation region, we conducted a speckle interferometric survey of 614 association members more massive than 0.4 {{ \mathcal M }} (spectral types earlier than M3V) based on the list of Luhman et al. (2018). We resolved 187 pairs, 55 of which are new …

2020 The Astronomical Journal
Gaia 23
Asymmetric expansion of coronal mass ejections in the low corona
DOI: 10.1051/0004-6361/201936664 Bibcode: 2020A&A...635A.100C

Cremades, H.; Iglesias, F. A.; Merenda, L. A.


Aims: Understanding how magnetic fields are structured within coronal mass ejections (CMEs), and how they evolve from the low corona into the heliosphere, is a major challenge for space weather forecasting and for solar physics. The study of CME morphology is a particularly auspicious approach to this problem, given that it holds a close rela…

2020 Astronomy and Astrophysics
SOHO 23
Vetting the optical transient candidates detected by the GWAC network using convolutional neural networks
DOI: 10.1093/mnras/staa2046 Bibcode: 2020MNRAS.497.2641T

Bertin, E.; Xu, Y.; Leroy, N. +11 more

The observation of the transient sky through a multitude of astrophysical messengers has led to several scientific breakthroughs in the last two decades, thanks to the fast evolution of the observational techniques and strategies employed by the astronomers. Now, it requires to be able to coordinate multiwavelength and multimessenger follow-up cam…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 23
The ASAS-SN catalogue of variable stars - VIII. 'Dipper' stars in the Lupus star-forming region
DOI: 10.1093/mnras/staa1588 Bibcode: 2020MNRAS.496.3257B

Kochanek, C. S.; Stanek, K. Z.; Shappee, B. J. +9 more

Some young stellar objects such as T Tauri-like 'dipper' stars vary due to transient partial occultation by circumstellar dust, and observations of this phenomenon inform us of conditions in the planet-forming zones close to these stars. Although many dipper stars have been identified with space missions such as Kepler/K2, ground-based telescopes …

2020 Monthly Notices of the Royal Astronomical Society
Gaia 23
Tracing the anemic stellar halo of M 101
DOI: 10.1051/0004-6361/201936994 Bibcode: 2020A&A...637A...8J

Bell, Eric F.; Holwerda, Benne W.; Monachesi, Antonela +3 more

Models of galaxy formation in a cosmological context predict that massive disk galaxies should have structured extended stellar halos. Recent studies in integrated light, however, report that a few galaxies, including the nearby disk galaxy M 101, have no measurable stellar halos to the detection limit. We aim to quantify the stellar content and s…

2020 Astronomy and Astrophysics
eHST 23
Direct Measurement of the Solar-wind Taylor Microscale Using MMS Turbulence Campaign Data
DOI: 10.3847/1538-4357/ab9ebe Bibcode: 2020ApJ...899...63B

Strangeway, Robert J.; Russell, Christopher T.; Chasapis, Alexandros +7 more

Using the novel Magnetospheric Multiscale (MMS) mission data accumulated during the 2019 MMS Solar Wind Turbulence Campaign, we calculate the Taylor microscale (λT) of the turbulent magnetic field in the solar wind. The Taylor microscale represents the onset of dissipative processes in classical turbulence theory. However, an accurate e…

2020 The Astrophysical Journal
Cluster 23
Plasma characterization at comet 67P between 2 and 4 AU from the Sun with the RPC-MIP instrument
DOI: 10.1051/0004-6361/202037571 Bibcode: 2020A&A...638A.124W

Henri, Pierre; Vallières, Xavier; Deca, Jan +2 more

The plasma of comet 67P/Churyumov-Gerasimenko is analyzed based on the RPC-MIP mutual impedance probe data of the Rosetta mission. Numerical simulations of the RPC-MIP instrumental response considering two populations of electrons were fit on experimental responses acquired from January to September 2016 to extract the electron densities and tempe…

2020 Astronomy and Astrophysics
Rosetta 23
A multi-chord stellar occultation by the large trans-Neptunian object (174567) Varda
DOI: 10.1051/0004-6361/202038526 Bibcode: 2020A&A...643A.125S

Berthier, J.; Carry, B.; Souami, D. +41 more

Context. We present results from the first recorded stellar occultation by the large trans-Neptunian object (174567) Varda that was observed on September 10, 2018. Varda belongs to the high-inclination dynamically excited population, and has a satellite, Ilmarë, which is half the size of Varda.
Aims: We determine the size and albedo of Varda …

2020 Astronomy and Astrophysics
Gaia eHST 23
Cloud Atlas: Weak Color Modulations Due to Rotation in the Planetary-mass Companion GU Psc b and 11 Other Brown Dwarfs
DOI: 10.3847/1538-3881/ab5f59 Bibcode: 2020AJ....159..125L

Schneider, Glenn; Apai, Dániel; Marley, Mark +10 more

Among the greatest challenges in understanding ultracool brown dwarf and exoplanet atmospheres is the evolution of cloud structure as a function of temperature and gravity. In this study, we present the rotational modulations of GU Psc b—a rare mid-T spectral type planetary-mass companion at the end of the L/T spectral type transition. Based on th…

2020 The Astronomical Journal
Gaia eHST 23