Search Publications

Detection of Periodicity in SiO Maser Intensity and Velocity Shift of the Symbiotic Star CH Cyg
DOI: 10.3847/2041-8213/ab9f99 Bibcode: 2020ApJ...897L..26C

Kim, Dong-Jin; Kim, Jaeheon; Cho, Se-Hyung +3 more

We performed simultaneous monitoring observations of H2O 616-523 and SiO V = 1, 2, $J=1\to $ 0, SiO V = 1, $J=2\to $ 1, $3\to 2$ maser lines toward the symbiotic star CH Cyg from 2012 December to 2019 November using the Korean very long baseline interferometry Network single-dish telescope. SiO V = 1, 2, $J=1\to 0$…

2020 The Astrophysical Journal
Gaia 0
Quasiperiodic Velocity Fluctuations in Eruptive Prominences Observed by AIA/SDO
DOI: 10.3847/1538-4357/ab7db6 Bibcode: 2020ApJ...893...40T

Tsvetkov, Tsvetan; Petrov, Nikola

The current study presents an investigation of the behavior of prominences during eruptions. Variations in the distribution of their velocities are detected at altitudes <0.6 R. Detailed analyses are carried out for 304 Å Solar Dynamics Observatory/Atmospheric Imaging Assembly (SDO/AIA) observations. To track the behavior of promine…

2020 The Astrophysical Journal
SOHO 0
Absolute Dimensions of the Unevolved F-type Eclipsing Binary BT Vulpeculae
DOI: 10.3847/1538-4357/ab85c6 Bibcode: 2020ApJ...894...96T

Torres, Guillermo; Fekel, Francis C.; Muterspaugh, Matthew W. +1 more

We report extensive differential V-band photometry and high-resolution spectroscopy for the 1.14 day, detached, double-lined eclipsing binary BT Vul (F0+F7). Our radial-velocity monitoring and light-curve analysis lead to absolute masses and radii of ${M}_{1}=1.5439\pm 0.0098\,{{ \mathcal M }}_{\odot }^{{\rm{N}}}$ and ${R}_{1}=1.536\pm 0.018\,{{ \…

2020 The Astrophysical Journal
Gaia 0
LSST: From Science Drivers to Reference Design and Anticipated Data Products
DOI: 10.3847/1538-4357/ab042c Bibcode: 2019ApJ...873..111I

Aubourg, Éric; Strauss, Michael A.; Anderson, Scott F. +324 more

We describe here the most ambitious survey currently planned in the optical, the Large Synoptic Survey Telescope (LSST). The LSST design is driven by four main science themes: probing dark energy and dark matter, taking an inventory of the solar system, exploring the transient optical sky, and mapping the Milky Way. LSST will be a large, wide-fiel…

2019 The Astrophysical Journal
Gaia 3899
Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics beyond ΛCDM
DOI: 10.3847/1538-4357/ab1422 Bibcode: 2019ApJ...876...85R

Casertano, Stefano; Riess, Adam G.; Yuan, Wenlong +2 more

We present an improved determination of the Hubble constant from Hubble Space Telescope (HST) observations of 70 long-period Cepheids in the Large Magellanic Cloud (LMC). These were obtained with the same WFC3 photometric system used to measure extragalactic Cepheids in the hosts of SNe Ia. Gyroscopic control of HST was employed to reduce overhead…

2019 The Astrophysical Journal
Gaia eHST 1873
PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter
DOI: 10.3847/2041-8213/ab50c5 Bibcode: 2019ApJ...887L..24M

Harding, A. K.; Ray, P. S.; Wood, K. S. +18 more

Neutron stars are not only of astrophysical interest, but are also of great interest to nuclear physicists because their attributes can be used to determine the properties of the dense matter in their cores. One of the most informative approaches for determining the equation of state (EoS) of this dense matter is to measure both a star’s equatoria…

2019 The Astrophysical Journal
XMM-Newton 1379
A 3D Dust Map Based on Gaia, Pan-STARRS 1, and 2MASS
DOI: 10.3847/1538-4357/ab5362 Bibcode: 2019ApJ...887...93G

Speagle, Joshua S.; Zucker, Catherine; Finkbeiner, Douglas +2 more

We present a new three-dimensional map of dust reddening, based on Gaia parallaxes and stellar photometry from Pan-STARRS 1 and 2MASS. This map covers the sky north of a decl. of -30°, out to a distance of a few kiloparsecs. This new map contains three major improvements over our previous work. First, the inclusion of Gaia parallaxes dramatically …

2019 The Astrophysical Journal
Gaia 1031
The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch
DOI: 10.3847/1538-4357/ab2f73 Bibcode: 2019ApJ...882...34F

Madore, Barry F.; Freedman, Wendy L.; Beaton, Rachael L. +10 more

We present a new and independent determination of the local value of the Hubble constant based on a calibration of the tip of the red giant branch (TRGB) applied to Type Ia supernovae (SNe Ia). We find a value of H 0 = 69.8 ± 0.8 (±1.1% stat) ± 1.7 (±2.4% sys) km s-1 Mpc-1. The TRGB method is both precise and accur…

2019 The Astrophysical Journal
Gaia eHST 748
The Optical to Mid-infrared Extinction Law Based on the APOGEE, Gaia DR2, Pan-STARRS1, SDSS, APASS, 2MASS, and WISE Surveys
DOI: 10.3847/1538-4357/ab1c61 Bibcode: 2019ApJ...877..116W

Wang, Shu; Chen, Xiaodian

A precise interstellar dust extinction law is critically important to interpret observations. There are two indicators of extinction: the color excess ratio (CER) and the relative extinction. Compared to the CER, the wavelength-dependent relative extinction is more challenging to be determined. In this work, we combine spectroscopic, astrometric, …

2019 The Astrophysical Journal
Gaia 379
The Circular Velocity Curve of the Milky Way from 5 to 25 kpc
DOI: 10.3847/1538-4357/aaf648 Bibcode: 2019ApJ...871..120E

Hogg, David W.; Rix, Hans-Walter; Ness, Melissa K. +1 more

We measure the circular velocity curve v c(R) of the Milky Way with the highest precision to date across Galactocentric distances of 5 ≤ R ≤ 25 kpc. Our analysis draws on the six-dimensional phase-space coordinates of ≳23,000 luminous red giant stars, for which we previously determined precise parallaxes using a data-driven model that c…

2019 The Astrophysical Journal
Gaia 355