Search Publications

High-resolution Spectroscopy of the GD-1 Stellar Stream Localizes the Perturber near the Orbital Plane of Sagittarius
DOI: 10.3847/2041-8213/ab800c Bibcode: 2020ApJ...892L..37B

Conroy, Charlie; Cargile, Phillip A.; Johnson, Benjamin D. +6 more

The 100° long thin stellar stream in the Milky Way halo, GD-1, has an ensemble of features that may be due to dynamical interactions. Using high-resolution MMT/Hectochelle spectroscopy we show that a spur of GD-1-like stars outside of the main stream are kinematically and chemically consistent with the main stream. In the spur, as in the main stre…

2020 The Astrophysical Journal
Gaia 53
SPCANet: Stellar Parameters and Chemical Abundances Network for LAMOST-II Medium Resolution Survey
DOI: 10.3847/1538-4357/ab6dea Bibcode: 2020ApJ...891...23W

Luo, A. -Li; Hou, Wen; Zhang, Shuo +6 more

The fundamental stellar atmospheric parameters (Teff and log g) and 13 chemical abundances are derived for medium-resolution spectroscopy from Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) Medium Resolution Survey (MRS) data sets with a deep-learning method. The neural networks we designed, named SPCANet, precisely …

2020 The Astrophysical Journal
Gaia 52
HST Proper Motions of NGC 147 and NGC 185: Orbital Histories and Tests of a Dynamically Coherent Andromeda Satellite Plane
DOI: 10.3847/1538-4357/abaf49 Bibcode: 2020ApJ...901...43S

van der Marel, Roeland P.; Geha, Marla; Fardal, Mark A. +4 more

We present the first proper-motion (PM) measurements for the dwarf elliptical galaxies NGC 147 and NGC 185, two satellite galaxies of M31, using multiepoch Hubble Space Telescope (HST) imaging data with time baselines of ∼8 yr. For each galaxy, we take an error-weighted average of measurements from HST Advanced Camera for Surveys/WFC and Wide Fiel…

2020 The Astrophysical Journal
eHST 51
GW Ori: Interactions between a Triple-star System and Its Circumtriple Disk in Action
DOI: 10.3847/2041-8213/ab8eb4 Bibcode: 2020ApJ...895L..18B

Dong, Ruobing; Kataoka, Akimasa; Takami, Michihiro +17 more

GW Ori is a hierarchical triple system with a rare circumtriple disk. We present Atacama Large Millimeter/submillimeter Array (ALMA) observations of 1.3 mm dust continuum and 12CO J = 2 - 1 molecular gas emission of the disk. For the first time, we identify three dust rings in the GW Ori disk at ∼46, 188, and 338 au, with estimated dust…

2020 The Astrophysical Journal
Gaia 51
Detection and Characterization of Oscillating Red Giants: First Results from the TESS Satellite
DOI: 10.3847/2041-8213/ab6443 Bibcode: 2020ApJ...889L..34S

Barclay, Thomas; Chaplin, William J.; Davies, Guy R. +78 more

Since the onset of the "space revolution" of high-precision high-cadence photometry, asteroseismology has been demonstrated as a powerful tool for informing Galactic archeology investigations. The launch of the NASA Transiting Exoplanet Survey Satellite (TESS) mission has enabled seismic-based inferences to go full sky—providing a clear advantage …

2020 The Astrophysical Journal
Gaia 51
Emergence of an Ultrared, Ultramassive Galaxy Cluster Core at z = 4
DOI: 10.3847/1538-4357/ab9d1f Bibcode: 2020ApJ...898..133L

Ivison, R. J.; Casey, Caitlin M.; Long, Arianna S. +6 more

Recent simulations and observations of massive galaxy cluster evolution predict that the majority of stellar mass buildup happens within cluster members by z = 2, before cluster virialization. Protoclusters rich with dusty, star-forming galaxies (DSFGs) at z > 3 are the favored candidate progenitors for these massive galaxy clusters at z ∼ 0. W…

2020 The Astrophysical Journal
Herschel eHST 51
Peter Pan Disks: Long-lived Accretion Disks Around Young M Stars
DOI: 10.3847/1538-4357/ab68e6 Bibcode: 2020ApJ...890..106S

Debes, John H.; Kuchner, Marc J.; Wisniewski, John P. +11 more

WISEA J080822.18-644357.3, an M star in the Carina association, exhibits extreme infrared excess and accretion activity at an age greater than the expected accretion disk lifetime. We consider J0808 as the prototypical example of a class of M star accretion disks at ages ≳20 Myr, which we call "Peter Pan" disks, because they apparently refuse to g…

2020 The Astrophysical Journal
Gaia 51
Sun-Heliosphere Observation-based Ionization Rates Model
DOI: 10.3847/1538-4357/ab99a4 Bibcode: 2020ApJ...897..179S

McComas, D. J.; Bzowski, M.; Tokumaru, M. +1 more

The solar wind (SW) and the extreme ultraviolet (EUV) radiation modulate fluxes of interstellar and heliospheric particles inside the heliosphere both in time and in space. Understanding this modulation is necessary to correctly interpret measurements of particles of interstellar origin inside the heliosphere. We present a revision of heliospheric…

2020 The Astrophysical Journal
SOHO Ulysses 50
Ion-neutral Interactions and Nonequilibrium Ionization in the Solar Chromosphere
DOI: 10.3847/1538-4357/ab643f Bibcode: 2020ApJ...889...95M

Martínez-Sykora, Juan; De Pontieu, Bart; Nóbrega-Siverio, Daniel +4 more

The thermal structure of the chromosphere is regulated through a complex interaction of various heating processes, radiative cooling, and the ionization degree of the plasma. Here, we study the impact on the thermal properties of the chromosphere when including the combined action of nonequilibrium ionization (NEI) of hydrogen and helium and ion-n…

2020 The Astrophysical Journal
IRIS 50
Spatially Resolved Ultraviolet Spectroscopy of the Great Dimming of Betelgeuse
DOI: 10.3847/1538-4357/aba516 Bibcode: 2020ApJ...899...68D

Dupree, Andrea K.; Guinan, Edward F.; Leike, Reimar +9 more

The bright supergiant Betelgeuse (Alpha Orionis, HD 39801) experienced a visual dimming during 2019 December and the first quarter of 2020, reaching an historic minimum 2020 February 7-13. During 2019 September-November, prior to the optical dimming event, the photosphere was expanding. At the same time, spatially resolved ultraviolet spectra usin…

2020 The Astrophysical Journal
eHST 50