Search Publications

Crepuscular Rays from the Highly Inclined Active Galactic Nucleus in IC 5063
DOI: 10.3847/2041-8213/abb9b6 Bibcode: 2020ApJ...902L..18M

Ho, Luis C.; Elvis, Martin; Barth, Aaron J. +10 more

On Earth near sunset, the Sun may cast "crepuscular rays" such that clouds near the horizon obscure the origin of light scattered in bright rays. In principle, active galactic nuclei (AGN) should be able to produce similar effects. Using new Hubble Space Telescope (HST) near-infrared and optical observations, we show that the active galaxy IC 5063…

2020 The Astrophysical Journal
eHST 9
Existence of the Metal-rich Stellar Halo and High-velocity Thick Disk in the Galaxy
DOI: 10.3847/1538-4357/abbd3d Bibcode: 2020ApJ...903..131Y

Shi, Jianrong; Ma, Jun; Du, Cuihua +3 more

Based on the second Gaia data release (DR2), combined with the LAMOST and APOGEE spectroscopic surveys, we study the kinematics and metallicity distribution of the high-velocity stars that have a relative speed of at least 220 $\mathrm{km}\ {{\rm{s}}}^{-1}$ with respect to the local standard of rest in the Galaxy. The rotational velocity distribut…

2020 The Astrophysical Journal
Gaia 9
Spectral Structures of Type II Solar Radio Bursts and Solar Energetic Particles
DOI: 10.3847/1538-4357/ab57ff Bibcode: 2020ApJ...888...50I

Yashiro, Seiji; Nitta, Nariaki V.; Iwai, Kazumasa +1 more

We investigated the relationship between the spectral structures of type II solar radio bursts in the hectometric and kilometric wavelength ranges and solar energetic particles (SEPs). To examine the statistical relationship between type II bursts and SEPs, we selected 26 coronal mass ejection (CME) events with similar characteristics (e.g., initi…

2020 The Astrophysical Journal
SOHO 9
Testing the Fidelity of Simulations of Black Hole-Galaxy Coevolution at z ∼ 1.5 with Observations
DOI: 10.3847/1538-4357/ab91be Bibcode: 2020ApJ...896..159D

Treu, Tommaso; Bhowmick, Aklant K.; Menci, N. +3 more

We examine the scaling relations between the mass of a supermassive black hole (SMBH) and its host galaxy properties at 1.2 < z <1.7 using both observational data and simulations. Recent measurements of 32 X-ray-selected, broad-line active galactic nuclei (AGNs) are compared with two independent state-of-the-art efforts, including the hydrod…

2020 The Astrophysical Journal
eHST 9
Mapping Circumstellar Magnetic Fields of Late-type Evolved Stars with the Goldreich-Kylafis Effect: CARMA Observations at λ1.3 mm of R Crt and R Leo
DOI: 10.3847/1538-4357/aba122 Bibcode: 2020ApJ...899..152H

Lai, Shih-Ping; Agudo, Iván; Vlemmings, Wouter H. T. +3 more

Mapping magnetic fields is the key to resolving the unclear physical picture of circumstellar magnetic fields in late-type evolved stars. Observations of linearly polarized emission from thermal molecular line transitions due to the Goldreich-Kylafis (G-K) effect provide valuable insights into the magnetic field geometry in these sources that are …

2020 The Astrophysical Journal
Gaia 9
Velocity Response of the Observed Explosive Events in the Lower Solar Atmosphere. I. Formation of the Flowing Cool-loop System
DOI: 10.3847/1538-4357/ab86bb Bibcode: 2020ApJ...894..155S

Tiwari, Sanjiv K.; Srivastava, A. K.; Konkol, P. +6 more

We observe plasma flows in cool loops using the Slit-Jaw Imager on board the Interface Region Imaging Spectrometer (IRIS). Huang et al. observed unusually broadened Si IV 1403 Šline profiles at the footpoints of such loops that were attributed to signatures of explosive events (EEs). We have chosen one such unidirectional flowing cool-loop system …

2020 The Astrophysical Journal
IRIS 9
Gemini Multi-Object Spectrograph Integral Field Unit Spectroscopy of the Double-peaked Broad Emission Line of a Red Active Galactic Nucleus
DOI: 10.3847/1538-4357/ab86a4 Bibcode: 2020ApJ...894..126K

Ho, Luis C.; Im, Myungshin; Kim, Minjin +1 more

Galaxy mergers are expected to produce multiple supermassive black holes (SMBHs) in close-separation, but the detection of such SMBHs has been difficult. 2MASS J165939.7 + 183436 is a red active galactic nucleus (AGN) that is a prospective merging SMBH candidate owing to its merging features in Hubble Space Telescope imaging and double-peaked broa…

2020 The Astrophysical Journal
eHST 9
The Advanced Spectral Library (ASTRAL): Abundance Analysis of the Chemically Peculiar Star HR 465
DOI: 10.3847/1538-4357/aba361 Bibcode: 2020ApJ...899..166N

Carpenter, Kenneth G.; Nielsen, Krister E.; Wahlgren, Glenn M. +1 more

This paper presents the results of the spectrum analysis of the B-type magnetic chemically peculiar star HR 465. HR 465 shows unusual abundance patterns that vary with a period of 21.5 yr. Our observations are recorded at φ = 0.45, 0.68, and 0.85 of the spectroscopic period, where φ = 0 represents the phase of maximum flux in the photometric y-ban…

2020 The Astrophysical Journal
eHST 9
A Mechanistic Study on the Formation of Acetic Acid (CH3COOH) in Polar Interstellar Analog Ices Exploiting Photoionization Reflectron Time-of-flight Mass Spectrometry
DOI: 10.3847/1538-4357/abafa4 Bibcode: 2020ApJ...901...84K

Kleimeier, N. Fabian; Eckhardt, André K.; Kaiser, Ralf I.

Acetic acid (CH3COOH) is considered a key molecule in the formation of the simplest amino acid, glycine, and consequently peptides. It is ubiquitous in the interstellar medium and has been detected toward hot cores, in the coma of comets, and on the surface of the comet 67P/Churyumov-Gerasimenko by the Rosetta mission. Here we present t…

2020 The Astrophysical Journal
Rosetta 9
Multiepoch VLBI of L Dwarf Binary 2MASS J0746+2000AB: Precise Mass Measurements and Confirmation of Radio Emission from Both Components
DOI: 10.3847/1538-4357/ab9177 Bibcode: 2020ApJ...897...11Z

Hallinan, Gregg; Zhang, Qicheng; Golden, Aaron +2 more

Surveys have shown that up to 1/10th of all ultracool dwarfs (UCDs) are appreciable radio emitters, with their emission attributed to a combination of gyrosynchrotron radiation and the electron cyclotron maser instability. 2M J0746+2000AB is a close stellar binary comprised of an L0 and L1.5 dwarf that was previously identified as a source of 5 GH…

2020 The Astrophysical Journal
Gaia 9