Search Publications

The Improved Orbit Solution and Component Masses of bet LMi
DOI: 10.3847/1538-3881/aba7bd Bibcode: 2020AJ....160..141W

Wang, Xiaoli; Fu, Yanning; Xia, Fang

bet LMi is a double-lined visual binary with an orbital period of ∼39 yr. Via a simultaneous fitting to both astrometric and radial velocity measurements, we give a complete and improved orbit solution with high precision. Then, the component masses are precisely determined as 2.98 ± 0.10 M and 1.92 ± 0.04 M with a relative…

2020 The Astronomical Journal
Hipparcos 1
A New Moving Group in the Local Arm
DOI: 10.3847/1538-3881/ab7fa9 Bibcode: 2020AJ....159..196L

Zhao, Gang; Chen, Yuqin; Zhao, Jingkun +5 more

We present a new moving group clustered in kinematics, spatial position, and elemental abundances. Its spatial position is around the center of the Local Arm of the Milky Way. A convergent point method was taken to select candidate member stars. Among 206 candidate member stars, 74 are pre-main-sequence stars and some of them have stellar disks. W…

2020 The Astronomical Journal
Gaia 1
Serendipitous Discovery of a Physical Binary Quasar at z = 1.76
DOI: 10.3847/1538-3881/ab6e67 Bibcode: 2020AJ....159..122A

Geier, S.; Fynbo, J. P. U.; Heintz, K. E. +7 more

Binary quasars are extremely rare objects, used to investigate clustering on very small scales at different redshifts. The cases where the two quasar components are gravitationally bound, known as physical binary quasars, can also exhibit enhanced astrophysical activity and therefore are of particular scientific interest. Here we present the seren…

2020 The Astronomical Journal
Gaia 1
KR Persei, a Mid-F Eclipsing Binary with a One-day Period
DOI: 10.3847/1538-3881/ab9094 Bibcode: 2020AJ....160...13S

Fekel, Francis C.; Muterspaugh, Matthew W.; Sowell, James R. +5 more

KR Per is a partially eclipsing binary with an orbital period of 0.9960798 days, very close to one sidereal day, making it difficult to obtain extensive phase coverage in a reasonable amount of time. We used the Wilson-Devinney program to determine its orbital elements and stellar absolute dimensions from recently acquired radial velocities and di…

2020 The Astronomical Journal
Gaia 0
Analytic Marginalization of Absorption Line Continua
DOI: 10.3847/1538-3881/ab602c Bibcode: 2020AJ....159...64T

Tchernyshyov, Kirill

Absorption line spectroscopy is a powerful way of measuring properties of stars and the interstellar medium. Absorption spectra are often analyzed manually, an approach that limits reproducibility and which cannot practically be applied to modern data sets consisting of thousands or even millions of spectra. Simultaneous probabilistic modeling of …

2020 The Astronomical Journal
eHST 0