Search Publications

Gravitational-wave Radiation of Double Degenerates with Extremely Low-mass White Dwarf Companions
DOI: 10.3847/1538-4357/ab7dc2 Bibcode: 2020ApJ...893....2L

Han, Zhanwen; Chen, Xuefei; Li, Zhenwei +3 more

Double degenerate (DD) systems are supposed to be significant gravitational-wave (GW) sources for future space-based GW detectors, e.g., the Laser Interferometer Space Antenna (LISA). Recently, one type of DD system with extremely low-mass WD (ELM WD; ≲ 0.30 M) companions was found in the ELM Survey. These companions have very short or…

2020 The Astrophysical Journal
Gaia 31
The Lyman Alpha Reference Sample. X. Predicting Lyα Output from Star-forming Galaxies Using Multivariate Regression
DOI: 10.3847/1538-4357/ab7a91 Bibcode: 2020ApJ...892...48R

Hayes, Matthew; Östlin, Göran; Melinder, Jens +4 more

Understanding the production and escape of Lyα radiation from star-forming galaxies is a long-standing problem in astrophysics. The ability to predict the Lyα luminosity of galaxies would open up new ways of exploring the epoch of reionization (EOR) and estimating Lyα emission from galaxies in cosmological simulations where radiative transfer calc…

2020 The Astrophysical Journal
eHST 30
Astrophysical Distance Scale. II. Application of the JAGB Method: A Nearby Galaxy Sample
DOI: 10.3847/1538-4357/aba9d8 Bibcode: 2020ApJ...899...67F

Madore, Barry F.; Freedman, Wendy L.

We apply the near-infrared J-region asymptotic giant branch (JAGB) method, recently introduced by Madore & Freedman, to measure the distances to 14 nearby galaxies out to 4 Mpc. We use the geometric detached eclipsing binary (DEB) distances to the LMC and SMC as independent zero-point calibrators. We find excellent agreement with previously pu…

2020 The Astrophysical Journal
eHST 30
Ionized and Atomic Interstellar Medium in the z = 6.003 Quasar SDSS J2310+1855
DOI: 10.3847/1538-4357/ababac Bibcode: 2020ApJ...900..131L

Fan, Xiaohui; Neri, Roberto; Menten, Karl M. +13 more

Observing the interstellar medium (ISM) in the z ≳ 6 quasar host galaxies is essential for understanding the coevolution between supermassive black holes and their hosts. To probe the gas physical conditions and search for imprints of active galactic nuclei (AGNs) on the ISM, we report ALMA observations of the [N II]122 µm and [O …

2020 The Astrophysical Journal
eHST 30
Exploring the Origin of Moving Groups and Diagonal Ridges by Simulations of Stellar Orbits and Birthplaces
DOI: 10.3847/1538-4357/ab59d1 Bibcode: 2020ApJ...888...75B

Pérez-Villegas, Angeles; Barros, Douglas A.; Michtchenko, Tatiana A. +2 more

The present paper is the culmination of a series aimed at contributing to the understanding of the kinematic structures of the solar neighborhood (SN), explaining the origin of the Local Arm, and relating the moving groups with the spiral-arms resonances in the disk. With a model for the Galactic potential, with the Sun inside the spiral corotatio…

2020 The Astrophysical Journal
Gaia 30
Balmer Break Galaxy Candidates at z ∼ 6: A Potential View on the Star Formation Activity at z ≳ 14
DOI: 10.3847/1538-4357/ab6596 Bibcode: 2020ApJ...889..137M

Ono, Yoshiaki; Fujimoto, Seiji; Harikane, Yuichi +15 more

We search for galaxies with a strong Balmer break (Balmer break galaxies; BBGs) at z ∼ 6 over a 0.41 deg2 effective area in the COSMOS field. Based on rich imaging data, including data obtained with the Atacama Large Millimeter/submillimeter Array (ALMA), three candidates are identified by their extremely red K-[3.6] colors, as well as …

2020 The Astrophysical Journal
Herschel eHST 30
From Nuclear to Circumgalactic: Zooming in on AGN-driven Outflows at z ∼ 2.2 with SINFONI
DOI: 10.3847/1538-4357/ab86ad Bibcode: 2020ApJ...894...28D

Lutz, D.; Wuyts, S.; Förster Schreiber, N. M. +16 more

We use deep adaptive optics assisted integral field spectroscopy from SINFONI on the VLT to study the spatially resolved properties of ionized gas outflows driven by active galactic nuclei (AGNs) in three galaxies at z ∼ 2.2—K20-ID5, COS4-11337, and J0901 + 1814. These systems probe AGN feedback from nuclear to circumgalactic scales and provide un…

2020 The Astrophysical Journal
Gaia eHST 30
Limits to Rest-frame Ultraviolet Emission from Far-infrared-luminous z ≃ 6 Quasar Hosts
DOI: 10.3847/1538-4357/abaa4c Bibcode: 2020ApJ...900...21M

Jahnke, K.; Koekemoer, A. M.; Fan, X. +20 more

We report on a Hubble Space Telescope search for rest-frame ultraviolet emission from the host galaxies of five far-infrared-luminous z ≃ 6 quasars and the z = 5.85 hot-dust-free quasar SDSS J0005-0006. We perform 2D surface brightness modeling for each quasar using a Markov Chain Monte Carlo estimator, to simultaneously fit and subtract the quasa…

2020 The Astrophysical Journal
eHST 30
Solving Grain Size Inconsistency between ALMA Polarization and VLA Continuum in the Ophiuchus IRS 48 Protoplanetary Disk
DOI: 10.3847/1538-4357/abaab4 Bibcode: 2020ApJ...900...81O

Henning, Thomas; Hull, Charles L. H.; Kataoka, Akimasa +6 more

The protoplanetary disk around Ophiuchus IRS 48 shows an azimuthally asymmetric dust distribution in (sub)millimeter observations, which is interpreted as a vortex, where millimeter/centimeter-sized particles are trapped at the location of the continuum peak. In this paper, we present 860 µm ALMA observations of polarized dust emission from …

2020 The Astrophysical Journal
Gaia 30
Runaway OB Stars in the Small Magellanic Cloud: Dynamical versus Supernova Ejections
DOI: 10.3847/1538-4357/abbc6b Bibcode: 2020ApJ...903...43D

Oey, M. S.; Castro, N.; Moe, M. +2 more

Runaway OB stars are ejected from their parent clusters via two mechanisms, both involving multiple stars: the dynamical ejection scenario (DES) and the binary supernova scenario (BSS). We constrain the relative contributions from these two ejection mechanisms in the Small Magellanic Cloud (SMC) using data for 304 field OB stars from the spatially…

2020 The Astrophysical Journal
Gaia 30