Search Publications

The Dual Role of Starbursts and Active Galactic Nuclei in Driving Extreme Molecular Outflows
DOI: 10.3847/1538-4357/aabccc Bibcode: 2018ApJ...859...35G

Bizzocchi, Luca; González-Alfonso, Eduardo; Darling, Jeremy +7 more

We report molecular gas observations of IRAS 20100-4156 and IRAS 03158+4227, two local ultraluminous infrared galaxies (ULIRGs) hosting some of the fastest and most massive molecular outflows known. Using Atacama Large Millimeter Array and Plateau de Bure Interferometer observations, we spatially resolve the CO (1-0) emission from the outflowing m…

2018 The Astrophysical Journal
eHST 29
On the Rate and on the Gravitational Wave Emission of Short and Long GRBs
DOI: 10.3847/1538-4357/aabee4 Bibcode: 2018ApJ...859...30R

Rodriguez, J.; Wang, Y.; Barres de Almeida, U. +13 more

On the ground of the large number of gamma-ray bursts (GRBs) detected with cosmological redshift, we classified GRBs in seven subclasses, all with binary progenitors which emit gravitational waves (GWs). Each binary is composed of combinations of carbon-oxygen cores (COcore), neutron stars (NSs), black holes (BHs), and white dwarfs (WDs…

2018 The Astrophysical Journal
INTEGRAL 29
RELICS: Strong Lensing Analysis of the Galaxy Clusters Abell S295, Abell 697, MACS J0025.4-1222, and MACS J0159.8-0849
DOI: 10.3847/1538-4357/aad2d3 Bibcode: 2018ApJ...863..145C

Ouchi, Masami; Mahler, Guillaume; Bradač, Maruša +37 more

We present a strong lensing analysis of four massive galaxy clusters imaged with the Hubble Space Telescope in the Reionization Lensing Cluster Survey. We use a light-traces-mass technique to uncover sets of multiple images and constrain the mass distribution of the clusters. These mass models are the first published for Abell S295 and MACS J0159.…

2018 The Astrophysical Journal
eHST 29
On the Dynamic Nature of a Quiescent Prominence Observed by IRIS and MSDP Spectrographs
DOI: 10.3847/1538-4357/aada08 Bibcode: 2018ApJ...865..123R

Schmieder, Brigitte; Chen, Yao; Labrosse, Nicolas +4 more

Quiescent solar prominences are generally considered to have a stable large-scale structure. However, they consist of multiple small-scale structures that are often significantly dynamic. To understand the nature of prominence plasma dynamics we use the high spatial, temporal, and spectral resolution observations obtained by Interface Region Imagi…

2018 The Astrophysical Journal
IRIS 29
The Temporal Development of Dust Formation and Destruction in Nova Sagittarii 2015#2 (V5668 SGR): A Panchromatic Study
DOI: 10.3847/1538-4357/aaba81 Bibcode: 2018ApJ...858...78G

Krautter, Joachim; Gehrz, R. D.; Shore, S. N. +15 more

We present 5-28 µm SOFIA FORECAST spectroscopy complemented by panchromatic X-ray through infrared observations of the CO nova V5668 Sgr documenting the formation and destruction of dust during ∼500 days following outburst. Dust condensation commenced by 82 days after outburst at a temperature of ∼1090 K. The condensation temperature indicat…

2018 The Astrophysical Journal
eHST 29
Anomalies in Time Delays of Lensed Gravitational Waves and Dark Matter Substructures
DOI: 10.3847/1538-4357/aae30f Bibcode: 2018ApJ...867...69L

Ding, Xuheng; Biesiada, Marek; Zhu, Zong-Hong +2 more

Cold dark matter scenarios of hierarchical large-scale structure formation predict the existence of abundant subhalos around large galaxies. However, the number of observed dwarf galaxies is far from this theoretical prediction, suggesting that most of the subhalos could be dark or quite faint. Gravitational lensing is a powerful tool to probe the…

2018 The Astrophysical Journal
eHST 29
Five New Globular Clusters Discovered in the Galactic Bulge
DOI: 10.3847/2041-8213/aacc68 Bibcode: 2018ApJ...860L..27C

Camargo, Denilso

This Letter reports the discovery of five new globular clusters (GCs) in the Galactic bulge (Camargo 1102, 1103, 1104, 1105, and 1106) using Wide-field Infrared Survey Explorer (WISE) images. Their natures are established by using 2MASS and Gaia second data release (DR2) photometry. The new findings are old and metal-poor GCs located less than 4 k…

2018 The Astrophysical Journal
Gaia 29
Chemical Inhomogeneities in the Pleiades: Signatures of Rocky-forming Material in Stellar Atmospheres
DOI: 10.3847/1538-4357/aad190 Bibcode: 2018ApJ...863..179S

Casey, Andrew R.; Meléndez, Jorge; Spina, Lorenzo +2 more

The aim of Galactic archaeology is to recover the history of our Galaxy through the information encoded in stars. An unprobed assumption of this field is that the chemical composition of a star is an immutable marker of the gas from which it formed. It is vital to test this assumption on open clusters, a group of stars formed from the same gas. Pr…

2018 The Astrophysical Journal
Gaia 29
The Distance to and the Near-infrared Extinction of the Monoceros Supernova Remnant
DOI: 10.3847/1538-4357/aaacd0 Bibcode: 2018ApJ...855...12Z

Jiang, Biwei; Zhao, He; Li, Jun +2 more

Supernova remnants (SNRs) contain information on the influence of supernova explosions on dust properties. Based on the color indices from the Two Micron All Sky Survey and the stellar parameters from the SDSS-DR12/Apache Point Observatory Galactic Evolution Experiment and LAMOST-DR2/LAMOST Experiment for Galactic Understanding and Exploration spe…

2018 The Astrophysical Journal
Gaia Herschel 29
Observations of the Kelvin-Helmholtz Instability Driven by Dynamic Motions in a Solar Prominence
DOI: 10.3847/2041-8213/aad9a5 Bibcode: 2018ApJ...864L..10H

Polito, Vanessa; Hillier, Andrew

Prominences are incredibly dynamic across the whole range of their observable spatial scales, with observations revealing gravity-driven fluid instabilities, waves, and turbulence. With all of these complex motions, it would be expected that instabilities driven by shear in the internal fluid motions would develop. However, evidence of these have …

2018 The Astrophysical Journal
IRIS 29