Search Publications

Luminosity Models and Density Profiles for Nuclear Star Clusters for a Nearby Volume-limited Sample of 29 Galaxies
DOI: 10.3847/1538-4357/abaaa7 Bibcode: 2020ApJ...900...32P

Pechetti, Renuka; Neumayer, Nadine; Kacharov, Nikolay +3 more

Nuclear star clusters (NSCs) are dense stellar clusters that are found at the centers of a majority of galaxies. In this paper, we study the density profiles for 29 galaxies in a volume-limited survey within 10 Mpc to characterize their NSCs. These galaxies span a 3 × 108-8 × 1010 M and a wide range of Hubble type…

2020 The Astrophysical Journal
eHST 45
A New Class of Roche Lobe-filling Hot Subdwarf Binaries
DOI: 10.3847/2041-8213/aba3c2 Bibcode: 2020ApJ...898L..25K

Duev, Dmitry A.; Szkody, Paula; Littlefair, S. P. +30 more

We present the discovery of the second binary with a Roche lobe-filling hot subdwarf transferring mass to a white dwarf (WD) companion. This 56 minute binary was discovered using data from the Zwicky Transient Facility. Spectroscopic observations reveal an He-sdOB star with an effective temperature of Teff = 33,700 ± 1000 K and a surfac…

2020 The Astrophysical Journal
Gaia 45
HAZMAT VI: The Evolution of Extreme Ultraviolet Radiation Emitted from Early M Stars
DOI: 10.3847/1538-4357/ab893a Bibcode: 2020ApJ...895....5P

Loyd, R. O. Parke; Peacock, Sarah; Barman, Travis +4 more

Quantifying the evolution of stellar extreme ultraviolet (EUV, 100-1000 Å) emission is critical for assessing the evolution of planetary atmospheres and the habitability of M dwarf systems. Previous studies from the HAbitable Zones and M dwarf Activity across Time (HAZMAT) program showed the far- and near-UV (FUV, NUV) emission from M stars at var…

2020 The Astrophysical Journal
Gaia eHST 45
SCExAO/CHARIS Direct Imaging Discovery of a 20 au Separation, Low-mass Ratio Brown Dwarf Companion to an Accelerating Sun-like Star
DOI: 10.3847/2041-8213/abc631 Bibcode: 2020ApJ...904L..25C

Currie, Thayne; Kwon, Jungmi; Tamura, Motohide +27 more

We present the direct imaging discovery of a substellar companion to the nearby Sun-like star, HD 33632 Aa, at a projected separation of ∼20 au, obtained with SCExAO/CHARIS integral field spectroscopy complemented by Keck/NIRC2 thermal infrared imaging. The companion, HD 33632 Ab, induces a 10.5σ astrometric acceleration on the star as detected wi…

2020 The Astrophysical Journal
Gaia Hipparcos 45
A Relationship between Stellar Age and Spot Coverage
DOI: 10.3847/1538-4357/ab79a0 Bibcode: 2020ApJ...893...67M

Morris, Brett M.

We investigate starspot distributions consistent with space-based photometry of F, G, and K stars in six stellar associations ranging in age from 10 Myr to 4 Gyr. We show that a simple light-curve statistic called the "smoothed amplitude" is proportional to stellar age as t-1/2, following a Skumanich-like spin-down relation. We marginal…

2020 The Astrophysical Journal
Gaia 45
A Deep CFHT Optical Search for a Counterpart to the Possible Neutron Star-Black Hole Merger GW190814
DOI: 10.3847/1538-4357/ab917d Bibcode: 2020ApJ...895...96V

Safi-Harb, Samar; Drout, Maria R.; Moon, Dae-Sik +10 more

We present a wide-field optical imaging search for electromagnetic counterparts to the likely neutron star-black hole (NS-BH) merger GW190814/S190814bv. This compact binary merger was detected through gravitational waves by the LIGO/Virgo interferometers, with masses suggestive of an NS-BH merger. We imaged the LIGO/Virgo localization region using…

2020 The Astrophysical Journal
Gaia 45
The Variable and Non-variable X-Ray Absorbers in Compton-thin Type II Active Galactic Nuclei
DOI: 10.3847/1538-4357/ab92ab Bibcode: 2020ApJ...897...66L

Nikutta, Robert; Laha, Sibasish; Markowitz, Alex G. +3 more

We have conducted an extensive X-ray spectral variability study of a sample of 20 Compton-thin type II galaxies using broadband spectra from XMM-Newton, Chandra, and Suzaku. The aim is to study the variability of the neutral intrinsic X-ray obscuration along the line of sight and investigate the properties and location of the dominant component of…

2020 The Astrophysical Journal
Suzaku XMM-Newton 44
Spitzer Follow-up of Extremely Cold Brown Dwarfs Discovered by the Backyard Worlds: Planet 9 Citizen Science Project
DOI: 10.3847/1538-4357/aba633 Bibcode: 2020ApJ...899..123M

Debes, John H.; Kiman, Rocio; Meisner, Aaron M. +38 more

We present Spitzer follow-up imaging of 95 candidate extremely cold brown dwarfs discovered by the Backyard Worlds: Planet 9 citizen science project, which uses visually perceived motion in multiepoch Wide-field Infrared Survey Explorer (WISE) images to identify previously unrecognized substellar neighbors to the Sun. We measure Spitzer [3.6]-[4.5…

2020 The Astrophysical Journal
Gaia 44
Detection of Strong Epicyclic Density Spikes in the GD-1 Stellar Stream: An Absence of Evidence for the Influence of Dark Matter Subhalos?
DOI: 10.3847/1538-4357/ab7303 Bibcode: 2020ApJ...891..161I

Martin, Nicolas; Malhan, Khyati; Famaey, Benoit +3 more

The density variations in thin stellar streams may encode important information on the nature of dark matter. For instance, if dark matter aggregates into massive subhalos, these perturbers are expected to scatter stars out of dynamically cold stellar streams, possibly leading to detectable gaps in those structures. Here, we reexamine the density …

2020 The Astrophysical Journal
Gaia 44
Ubiquitous Molecular Outflows in z > 4 Massive, Dusty Galaxies. I. Sample Overview and Clumpy Structure in Molecular Outflows on 500 pc Scales
DOI: 10.3847/1538-4357/abc47f Bibcode: 2020ApJ...905...85S

Gonzalez, Anthony H.; Phadke, Kedar A.; Aravena, Manuel +14 more

Massive galaxy-scale outflows of gas are one of the most commonly invoked mechanisms to regulate the growth and evolution of galaxies throughout the universe. While the gas in outflows spans a large range of temperatures and densities, the cold molecular phase is of particular interest because molecular outflows may be capable of suppressing star …

2020 The Astrophysical Journal
Herschel 44