Search Publications

Noncircular Motions in the Outer Perseus Spiral Arm
DOI: 10.3847/1538-4357/ab12e0 Bibcode: 2019ApJ...876...30S

Menten, Karl M.; Reid, Mark J.; Sakai, Nobuyuki +2 more

We report measurements of parallax and proper motion for five 6.7 GHz methanol maser sources in the outer regions of the Perseus arm as part of the BeSSeL Survey of the Galaxy. By combining our results with previous astrometric results, we determine an average spiral arm pitch angle of 9.°2 ± 1.°5 and an arm width of 0.39 kpc for this spiral arm. …

2019 The Astrophysical Journal
Gaia 21
Signatures of Tidal Disruption in Ultra-faint Dwarf Galaxies: A Combined HST, Gaia, and MMT/Hectochelle Study of Leo V
DOI: 10.3847/1538-4357/ab45ec Bibcode: 2019ApJ...885...53M

Caldwell, Nelson; Strader, Jay; Seth, Anil C. +10 more

The ultra-faint dwarf galaxy Leo V has shown both photometric overdensities and kinematic members at large radii, along with a tentative kinematic gradient, suggesting that it may have undergone a close encounter with the Milky Way. We investigate these signs of disruption through a combination of (i) high precision photometry obtained with the Hu…

2019 The Astrophysical Journal
Gaia eHST 21
Resolved Molecular Gas and Star Formation Properties of the Strongly Lensed z = 2.26 Galaxy SDSS J0901+1814
DOI: 10.3847/1538-4357/ab22b9 Bibcode: 2019ApJ...879...52S

Wilner, David J.; Keeton, Charles R.; Lutz, Dieter +8 more

We present ∼1″ resolution (∼2 kpc in the source plane) observations of the CO (1-0), CO (3-2), Hα, and [N II] lines in the strongly lensed z = 2.26 star-forming galaxy SDSS J0901+1814. We use these observations to constrain the lensing potential of a foreground group of galaxies, and our source-plane reconstructions indicate that SDSS J0901+1814 i…

2019 The Astrophysical Journal
eHST 21
Identifying Galactic Halo Substructure in 6D Phase Space Using ∼13,000 LAMOST K Giants
DOI: 10.3847/1538-4357/ab2462 Bibcode: 2019ApJ...880...65Y

Tian, Hao; Zhao, Gang; Li, Chengdong +6 more

We construct a large halo K-giant sample by combining the positions, distances, radial velocities, and metallicities of over 13,000 LAMOST DR5 halo K giants with the Gaia DR2 proper motions, which covers a Galactocentric distance range of 5-120 kpc. Using a position-velocity clustering estimator (the 6Distance), we statistically quantify the prese…

2019 The Astrophysical Journal
Gaia 21
TESS Habitable Zone Star Catalog
DOI: 10.3847/2041-8213/ab0e8d Bibcode: 2019ApJ...874L...8K

Stassun, K.; Kaltenegger, L.; Pepper, J. +1 more

We present the Transiting Exoplanet Survey Satellite (TESS) Habitable Zone Stars Catalog, a list of 1822 nearby stars with a TESS magnitude brighter than T = 12 and reliable distances from Gaia DR2, around which the NASA’s TESS mission can detect transiting planets, which receive Earth-like irradiation. For all those stars TESS is sensitive down t…

2019 The Astrophysical Journal
Gaia 21
The Unexpected Spectrum of the Innermost Ejecta of the Red Hypergiant VY CMa
DOI: 10.3847/2041-8213/ab11e5 Bibcode: 2019ApJ...874L..26H

Humphreys, Roberta M.; Jones, Terry J.; Gordon, Michael S. +6 more

Hubble Space Telescope/STIS spectra of the small clumps and filaments closest to the central star in VY CMa reveal that the very strong K I emission and TiO and VO molecular emission, long thought to form in a dusty circumstellar shell, actually originate in a few small clumps hundreds of au from the star. The K I lines are 10-20 times stronger in…

2019 The Astrophysical Journal
eHST 21
Multiwavelength Period-Luminosity and Period-Luminosity-Color Relations at Maximum Light for Mira Variables in the Magellanic Clouds
DOI: 10.3847/1538-4357/ab38c2 Bibcode: 2019ApJ...884...20B

Matsunaga, Noriyuki; de Grijs, Richard; Rejkuba, Marina +8 more

We present Period-Luminosity and Period-Luminosity-Color relations at maximum light for Mira variables in the Magellanic Clouds using time-series data from the Optical Gravitational Lensing Experiment (OGLE-III) and Gaia data release 2. The maximum-light relations exhibit a scatter typically up to ∼30% smaller than their mean-light counterparts. T…

2019 The Astrophysical Journal
Gaia 21
Asymmetric Drift in the Andromeda Galaxy (M31) as a Function of Stellar Age
DOI: 10.3847/1538-4357/aaf1ba Bibcode: 2019ApJ...871...11Q

Williams, Benjamin F.; Gilbert, Karoline M.; Chemin, Laurent +5 more

We analyze the kinematics of Andromeda’s disk as a function of stellar age by using photometry from the Panchromatic Hubble Andromeda Treasury survey and spectroscopy from the Spectroscopic and Photometric Landscape of Andromeda’s Stellar Halo survey. We use H I 21 cm and CO (J=1\to 0) data to examine the difference between the deprojected rotatio…

2019 The Astrophysical Journal
eHST 21
The R-Process Alliance: Discovery of a Low-α, r-process-enhanced Metal-poor Star in the Galactic Halo
DOI: 10.3847/1538-4357/ab0c02 Bibcode: 2019ApJ...874..148S

Grebel, Eva K.; Steinmetz, Matthias; Beers, Timothy C. +24 more

A new moderately r-process-enhanced metal-poor star, RAVE J093730.5-062655, has been identified in the Milky Way halo as part of an ongoing survey by the R-Process Alliance. The temperature and surface gravity indicate that J0937-0626 is likely a horizontal branch star. At [Fe/H] = -1.86, J0937-0626 is found to have subsolar [X/Fe] ratios for near…

2019 The Astrophysical Journal
Gaia 21
Bidirectional Reconnection Outflows in an Active Region
DOI: 10.3847/1538-4357/ab3657 Bibcode: 2019ApJ...883...52R

Aulanier, Guillaume; Schmieder, Brigitte; Masson, Sophie +4 more

We report on bidirectional coronal reconnection outflows reaching ±200 km s-1 as observed in an active region with the Si IV and C II spectra of the Interface Region Imaging Spectrograph (IRIS). The evolution of the active region with an emerging flux, a failed filament eruption, and a jet is followed in Solar Dynamical Observatory (SDO…

2019 The Astrophysical Journal
IRIS 21