Search Publications

Galactic Rotation and the Oort Constants in the Solar Vicinity
DOI: 10.3847/1538-4357/ab0104 Bibcode: 2019ApJ...872..205L

Zhao, Gang; Li, Chengdong; Yang, Chengqun

Gaia DR2 data are used to calculate the Oort constants and derive the Galactic rotational properties in this work. We choose the solar vicinity stars with a “clean” sample within 500 pc. The Oort constants are then fitted through the relation between the proper motions as a function of Galactic longitude l. A maximum likelihood method is adopted t…

2019 The Astrophysical Journal
Gaia 26
Spectral and Timing Analysis of the Accretion-powered Pulsar 4U 1626-67 Observed with Suzaku and NuSTAR
DOI: 10.3847/1538-4357/ab1f87 Bibcode: 2019ApJ...878..121I

Enoto, Teruaki; Chakrabarty, Deepto; Terada, Yukikatsu +13 more

We present an analysis of the spectral shape and pulse profile of the accretion-powered pulsar 4U 1626-67 observed with Suzaku and Nuclear Spectroscopic Telescope Array (NuSTAR) during a spin-up state. The pulsar, which experienced a torque reversal to spin-up in 2008, has a spin period of ∼7.7 s. Comparing the phase-averaged spectra obtained with…

2019 The Astrophysical Journal
Suzaku 26
Distances to Galactic OB Stars: Photometry versus Parallax
DOI: 10.3847/1538-4357/ab357d Bibcode: 2019ApJ...882..180S

Shull, J. Michael; Danforth, Charles W.

For application to surveys of interstellar matter and Galactic structure, we compute new spectrophotometric distances to 139 OB stars frequently used as background targets for UV spectroscopy. Many of these stars have updated spectral types and digital photometry with reddening corrections from the Galactic O-Star (GOS) spectroscopic survey. We co…

2019 The Astrophysical Journal
Gaia 26
On the Origin of Solar Torsional Oscillations and Extended Solar Cycle
DOI: 10.3847/1538-4357/ab5952 Bibcode: 2019ApJ...887..215P

Kosovichev, A. G.; Pipin, V. V.

We present a nonlinear mean-field model of the solar interior dynamics and dynamo, which reproduces the observed cyclic variations of the global magnetic field of the Sun, as well as the differential rotation and meridional circulation. Using this model, we explain, for the first time, the extended 22 yr pattern of the solar torsional oscillations…

2019 The Astrophysical Journal
SOHO 26
Detecting Thin Stellar Streams in External Galaxies: Resolved Stars and Integrated Light
DOI: 10.3847/1538-4357/ab3e06 Bibcode: 2019ApJ...883...87P

Williams, Benjamin F.; Ibata, Rodrigo A.; Johnston, Kathryn V. +3 more

The morphology of thin stellar streams can be used to test the nature of dark matter. It is therefore crucial to extend searches for globular cluster (GC) streams to other galaxies than the Milky Way. In this paper, we investigate the current and future prospects of detecting GC streams in external galaxies in resolved stars (e.g., with Wide Field…

2019 The Astrophysical Journal
Gaia 26
Stellar Mass Growth of Brightest Cluster Galaxy Progenitors in COSMOS Since z ∼ 3
DOI: 10.3847/1538-4357/ab30c9 Bibcode: 2019ApJ...881..150C

Casey, Caitlin M.; Kartaltepe, Jeyhan S.; Le Fèvre, Olivier +5 more

We examine the role of environment on the in situ star formation (SF) hosted by the progenitors of the most massive galaxies in the present-day universe, the brightest cluster galaxies (BCGs), from z ∼ 3 to present in the COSMOS field. Progenitors are selected from the COSMOS field using a stellar mass cut motivated by the evolving cumulative como…

2019 The Astrophysical Journal
Herschel eHST 26
An Enormous Molecular Gas Flow in the RX J0821+0752 Galaxy Cluster
DOI: 10.3847/1538-4357/aaf1b4 Bibcode: 2019ApJ...870...57V

Fabian, A. C.; Combes, F.; McDonald, M. +6 more

We present recent Chandra X-ray observations of the RX J0821.0+0752 galaxy cluster, in addition to ALMA observations of the CO(1-0) and CO(3-2) line emission tracing the molecular gas in its central galaxy. All of the CO line emission, originating from a {10}10 {M} molecular gas reservoir, is located several kiloparsecs awa…

2019 The Astrophysical Journal
eHST 26
The Planet Formation Potential around a 45 Myr Old Accreting M Dwarf
DOI: 10.3847/1538-4357/aaf794 Bibcode: 2019ApJ...872...92F

Hughes, A. Meredith; Murphy, Simon J.; Mamajek, Eric E. +1 more

Debris disk detections around M dwarfs are rare, and so far no gas emission has been detected from an M dwarf debris disk. This makes the 45 Myr old M dwarf WISE J080822.18-644357.3 a bit of a curiosity; it has a strong infrared excess at an age beyond the lifetime of a typical planet-forming disk, and also exhibits broad Hα emission consistent wi…

2019 The Astrophysical Journal
Gaia 26
ALMA Observations of Atomic Carbon [C I] ( 3 P 1 3 P 0 ) and Low-J CO Lines in the Starburst Galaxy NGC 1808
DOI: 10.3847/1538-4357/ab55dc Bibcode: 2019ApJ...887..143S

Seta, Masumichi; Salak, Dragan; Nakai, Naomasa +1 more

We present [C I] ≤ft({}3{{P}}1\to {}3{{P}}0\right), 12CO, 13CO, and C18O (J=2\to 1) observations of the central region (radius 1 kpc) of the starburst galaxy NGC 1808 at 30-50 pc resolution conducted with the Atacama Large Millimeter/submillimeter Array. Radiative transfe…

2019 The Astrophysical Journal
eHST 26
The Precious Set of Radio-optical Reference Frame Objects in the Light of Gaia DR2 Data
DOI: 10.3847/1538-4357/aafa1c Bibcode: 2019ApJ...873..132M

Schmitt, Henrique R.; Makarov, Valeri V.; Berghea, Ciprian T. +2 more

We investigate a sample of 3413 International Celestial Reference Frame (ICRF3) extragalactic radio-loud sources with accurate positions determined by very long baseline interferometry in the S/X band, mostly active galactic nuclei and quasars, which are cross-matched with optical sources in the second Gaia data release (Gaia DR2). The main goal o…

2019 The Astrophysical Journal
Gaia 26