Search Publications

Radial Velocities of Low-mass Candidate TWA Members
DOI: 10.3847/1538-4357/ab2591 Bibcode: 2019ApJ...879...63K

Mace, Gregory; Sokal, Kimberly; Kidder, Benjamin +2 more

Nearby young moving groups provide unique samples of similar age stars for testing the evolution of physical properties. Incomplete and/or incorrect group membership classifications reduce the usefulness of the group, which we assume to be coeval. With near-infrared spectra of two candidate members of the TW Hya Association, 2MASS J12354615-411553…

2019 The Astrophysical Journal
Gaia 1
Detection of Crystalline and Fine-grained Calcic Plagioclases on Vesta
DOI: 10.3847/2041-8213/ab339e Bibcode: 2019ApJ...882L..22P

Aoki, S.; Oliva, F.; D'Aversa, E. +8 more

Plagioclase feldspars are among the most prevalent minerals in the solar system, and are present in many chondritic and achondritic meteorite families. Nevertheless, spectral features of plagioclases have never been unambiguously and directly observed in remote observations of asteroids. We report here the detection of an absorption band at 12.2 &…

2019 The Astrophysical Journal
ISO 1
A Hint of Three-section Halo As Seen from the APOGEE DR14
DOI: 10.3847/1538-4357/aaf80f Bibcode: 2019ApJ...871..216C

Zhao, G.; Chen, Y. Q.; Xue, X. X. +4 more

Based on the [M/H] versus [Mg/Fe] diagram and distances from APOGEE data release 14, we compare the spatial distributions, the l - V los diagram, and the abundance gradients between high-[Mg/Fe] and low-[Mg/Fe] sequences. The two sequences are clearly shown at 5< | Z| < 10 {kpc} in the metallicity range of -1.6 < [M/H] < -0.…

2019 The Astrophysical Journal
Gaia 1
Estimates of the Atmospheric Escape Rates of CH4 from Titan
DOI: 10.3847/1538-4357/ab1d59 Bibcode: 2019ApJ...878....3H

Ip, Wing-Huen; Hsu, Jen-Kai

The upper atmosphere of Titan is highly variable as characterized by the variations of the thermospheric and exospheric temperatures from in situ measurements by Cassini at different Titan encounters. A related question has to do with the escape flux of CH4 that might also change with the complex plasma environment and ionospheric condi…

2019 The Astrophysical Journal
Cassini 1
Opposite Polarity Magnetic Fields and Convective Downflows in a Simulated Sunspot Penumbra
DOI: 10.3847/1538-4357/ab3c6b Bibcode: 2019ApJ...884...94B

Rempel, Matthias; Bharti, Lokesh

Recent numerical simulations and observations of sunspots show a significant amount of opposite polarity magnetic fields within the sunspot penumbra. Most of the opposite polarity fields are associated with convective downflows. We present an analysis of 3D MHD simulations through forward modeling of synthetic Stokes profiles of the Fe I 6301.5 Å …

2019 The Astrophysical Journal
Hinode 1
Effect of the Surface Roughness of Icy Grains on Molecular Oxygen Chemistry in Molecular Clouds
DOI: 10.3847/1538-4357/ab3400 Bibcode: 2019ApJ...882..131M

Gunell, H.; De Keyser, J.; Mousis, O. +6 more

Molecular cloud and protosolar nebula chemistry involves a strong interaction between the gas phase and the surface of icy grains. The exchanges between the gas phase and the solid phase depend not only on the adsorption and desorption rates but also on the geometry of the surface of the grains. Indeed, for sufficient levels of surface roughness, …

2019 The Astrophysical Journal
Rosetta 0
Northern Galactic Molecular Cloud Clumps in Hi-GAL: Clump and Star Formation within Clouds
DOI: 10.3847/1538-4357/ab2e03 Bibcode: 2019ApJ...881...90Z

Rosolowsky, Erik; Zetterlund, Erika; Glenn, Jason

We investigate how the properties of Galactic giant molecular clouds (GMCs) and their denser substructures (clumps) correlate with the local star formation rate (SFR). We trace clouds using the 12CO(3-2) transition, as observed by the CO High Resolution Survey. We identify their constituent clumps using thermal dust emission, as observe…

2019 The Astrophysical Journal
Herschel 0
A Kinematically Cold Structure of Candidate Young OB Stars toward the Anticenter
DOI: 10.3847/1538-4357/ab36b8 Bibcode: 2019ApJ...883....8C

Casetti-Dinescu, Dana I.; Girard, Terrence M.

We combine Galaxy Evolution Explorer and Gaia DR2 catalogs to track star formation in the outskirts of our Galaxy. Using photometry, proper motions, and parallaxes we identify a structure of ∼300 OB-type candidates located between 12 and 15 kpc from the Galactic center that are kinematically cold. The structure is located between l = 120° and 200°…

2019 The Astrophysical Journal
Gaia 0
Probing the Bardeen-Petterson Effect in Tidal Disruption Events with Spectral line Reverberation Mapping
DOI: 10.3847/1538-4357/ab3e3e Bibcode: 2019ApJ...884...72Z

Dovčiak, Michal; Zhang, Wenda; Karas, Vladimír +1 more

For an inclined accretion flow around a rotating black hole, the combined effect of the Lense-Thirring precession and viscous torque tends to align the inner part of the flow with the black hole spin, leading to the formation of a warped disk, known as the Bardeen-Petterson (BP) effect. In tidal disruption events (TDEs) in which a supermassive bla…

2019 The Astrophysical Journal
XMM-Newton 0
Size Scaling of Clump Instabilities in Turbulent, Feedback-regulated Disks
DOI: 10.3847/1538-4357/ab0b41 Bibcode: 2019ApJ...874..170A

Glazebrook, Karl; Fisher, Deanne B.; Obreschkow, Danail +5 more

We explore the scaling between the size of star-forming clumps and rotational support in massively star-forming galactic disks. The analysis relies on simulations of a clumpy galaxy at z = 2 and the observed DYnamics of Newly Assembled Massive Objects (DYNAMO) sample of rare clumpy analogs at z ≈ 0.1 to test a predictive clump size scaling propose…

2019 The Astrophysical Journal
eHST 0