Search Publications

High Gas Fraction in a CO-detected Main-sequence Galaxy at z > 3
DOI: 10.3847/1538-4357/ab0b3c Bibcode: 2019ApJ...875....6G

Daddi, Emanuele; Neri, Roberto; Dannerbauer, Helmut +3 more

We report NOrthern Extended Millimetre Array (NOEMA) observations of warm molecular gas traced by CO(5 - 4) in a z∼ 3.2 gas-rich main-sequence (MS) galaxy, initially serendipitously detected in CO(3 - 2) emission in “blind” deep NOEMA observations. Our target shows a gas excitation consistent with that seen in z∼ 1.5 MS galaxies ({L}CO(…

2019 The Astrophysical Journal
eHST 32
A High-resolution Mid-infrared Survey of Water Emission from Protoplanetary Disks
DOI: 10.3847/1538-4357/ab05c3 Bibcode: 2019ApJ...874...24S

Zhang, Ke; Lacy, John; Najita, Joan R. +5 more

We present the largest survey of spectrally resolved mid-infrared water emission to date, with spectra for 11 disks obtained with the Michelle and TEXES spectrographs on Gemini North. Water emission is detected in six of eight disks around classical T Tauri stars. Water emission is not detected in the transitional disks SR 24 N and SR 24 S, in spi…

2019 The Astrophysical Journal
Gaia 32
The ACS Fornax Cluster Survey. III. Globular Cluster Specific Frequencies of Early-type Galaxies
DOI: 10.3847/1538-4357/ab12d9 Bibcode: 2019ApJ...875..156L

Jordán, Andrés; Côté, Patrick; Peng, Eric W. +4 more

The globular cluster (GC) specific frequency (S N ), defined as the number of GCs per unit galactic luminosity, represents the efficiency of GC formation (and survival) compared to field stars. Despite the naive expectation that star cluster formation should scale directly with star formation, this efficiency varies widely across galax…

2019 The Astrophysical Journal
eHST 32
Implications of a Time-varying Galactic Potential for Determinations of the Dynamical Surface Density
DOI: 10.3847/2041-8213/ab25f3 Bibcode: 2019ApJ...879L..15H

Hernquist, Lars; Famaey, Benoit; Haines, Tim +2 more

We analyze a high-resolution N-body simulation of a live stellar disk perturbed by the recent passage of a massive dwarf galaxy that induces a wobble, in-plane rings, and phase spirals in the disk. The implications of the phase-space structures and the estimate of the matter density through traditional Jeans modeling are investigated. The dwarf sa…

2019 The Astrophysical Journal
Gaia 31
Observational Analysis on the Early Evolution of a CME Flux Rope: Preflare Reconnection and Flux Rope’s Footpoint Drift
DOI: 10.3847/1538-4357/ab527e Bibcode: 2019ApJ...887..118C

Yang, Jiayan; Ji, Kaifan; Duan, Yadan +1 more

We study the early evolution of a hot-channel-like magnetic flux rope (MFR) toward eruption. Combining with imaging observation and magnetic field extrapolation, we find that the hot channel possibly originated from a preexisting seed MFR with a hyperbolic flux tube (HFT). In the precursor phase, three-dimensional tether-cutting reconnection at th…

2019 The Astrophysical Journal
SOHO 31
The Formation Conditions of the Wide Binary Class 0 Protostars within BHR 71
DOI: 10.3847/1538-4357/aaef87 Bibcode: 2019ApJ...870...81T

Bourke, Tyler L.; Codella, Claudio; Chen, Xuepeng +7 more

We present a characterization of the binary protostar system that is forming within a dense core in the isolated dark cloud BHR71. The pair of protostars, IRS1 and IRS2, are both in the Class 0 phase, determined from observations that resolve the sources from 1 µm out to 250 µm and from 1.3 mm to 1.3 cm. The resolved observations enabl…

2019 The Astrophysical Journal
Herschel 31
A Secondary Fan-spine Magnetic Structure in Active Region 11897
DOI: 10.3847/1538-4357/aaf4f4 Bibcode: 2019ApJ...871....4H

Hou, Yijun; Li, Ting; Yang, Shuhong +1 more

Fan-spine is a special topology in solar atmosphere and is closely related to magnetic null point, as well as circular-ribbon flares, which can provide important information for understanding the intrinsic 3D nature of solar flares. However, the fine structure within the fan has rarely been investigated. In present paper, we investigate a secondar…

2019 The Astrophysical Journal
IRIS 31
Search for Gravitational-wave Signals Associated with Gamma-Ray Bursts during the Second Observing Run of Advanced LIGO and Advanced Virgo
DOI: 10.3847/1538-4357/ab4b48 Bibcode: 2019ApJ...886...75A

Lee, H. M.; Williams, D.; Hurley, K. +1196 more

We present the results of targeted searches for gravitational-wave transients associated with gamma-ray bursts during the second observing run of Advanced LIGO and Advanced Virgo, which took place from 2016 November to 2017 August. We have analyzed 98 gamma-ray bursts using an unmodeled search method that searches for generic transient gravitation…

2019 The Astrophysical Journal
INTEGRAL 31
Cloud Atlas: Rotational Spectral Modulations and Potential Sulfide Clouds in the Planetary-mass, Late T-type Companion Ross 458C
DOI: 10.3847/2041-8213/ab13b9 Bibcode: 2019ApJ...875L..15M

Schneider, Glenn; Apai, Dániel; Burgasser, Adam J. +11 more

Measurements of photometric variability at different wavelengths provide insights into the vertical cloud structure of brown dwarfs and planetary-mass objects. In seven Hubble Space Telescope consecutive orbits, spanning ∼10 hr of observing time, we obtained time-resolved spectroscopy of the planetary-mass T8 dwarf Ross 458 C using the near-infrar…

2019 The Astrophysical Journal
Gaia eHST 31
Multi-component Decomposition of Astronomical Spectra by Compressed Sensing
DOI: 10.3847/1538-4357/ab263d Bibcode: 2019ApJ...882...13C

Winebarger, Amy R.; Antolin, Patrick; Testa, Paola +9 more

The signal measured by an astronomical spectrometer may be due to radiation from a multi-component mixture of plasmas with a range of physical properties (e.g., temperature, Doppler velocity). Confusion between multiple components may be exacerbated if the spectrometer sensor is illuminated by overlapping spectra dispersed from different slits, wi…

2019 The Astrophysical Journal
Hinode 31