Search Publications

Unveiling short-period binaries in the inner VVV bulge
DOI: 10.1093/mnras/stab888 Bibcode: 2021MNRAS.504..654B

Minniti, D.; Contreras Ramos, R.; Saito, R. K. +5 more

Most of our knowledge of the structure of the Milky Way has come from the study of variable stars. Among these variables, mimicking the periodic variation of pulsating stars, are eclipsing binaries. These stars are important in astrophysics because they allow us to directly measure the radii and masses of the components, as well as the distance to…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 7
Element Abundance Analysis of the Metal-rich Stellar Halo and High-velocity Thick Disk in the Galaxy
DOI: 10.3847/1538-4357/abff52 Bibcode: 2021ApJ...915....9Z

Shi, Jianrong; Ma, Jun; Du, Cuihua +3 more

Based on the second Gaia data release (DR2) and APOGEE (DR16) spectroscopic surveys, we define two kinds of star samples: high-velocity thick disk (HVTD) with vφ > 90 km s-1 and metal-rich stellar halo (MRSH) with vφ < 90 km s-1. Due to high-resolution spectra data from APOGEE (DR16), we can accura…

2021 The Astrophysical Journal
Gaia 7
Investigation of the in-flight anomalies of the LISA Pathfinder Test Mass release mechanism
DOI: 10.1016/j.asr.2021.04.050 Bibcode: 2021AdSpR..68.2600B

Bortoluzzi, D.; Mendes, J.; Vignotto, D. +1 more

The LISA Pathfinder mission was flown to test some key technologies for the in-flight detection of gravitational waves. The mechanism developed to initialise the science phase, releasing the test mass into a geodesic trajectory, produced unexpected test mass states, requiring dedicated in-flight and on-ground test campaigns. Due to the limited inf…

2021 Advances in Space Research
LISAPathfinder 7
A spectroscopically confirmed Gaia-selected sample of 318 new young stars within ∼200 pc
DOI: 10.1093/mnras/stab513 Bibcode: 2021MNRAS.503..938Z

Zhou, George; Nordlander, Thomas; Žerjal, Maruša +7 more

In the Gaia era, the majority of stars in the Solar neighbourhood have parallaxes and proper motions precisely determined while spectroscopic age indicators are still missing for a large fraction of low-mass young stars. In this work, we select 756 overluminous late K and early M young star candidates in the southern sky and observe them over 64 n…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 7
Search for age pattern across spiral arms of the Milky Way
DOI: 10.1088/1674-4527/21/1/9 Bibcode: 2021RAA....21....9H

Xu, Ye; Hou, Li-Gang; He, Zhi-Hong

The age pattern across spiral arms is one of the key observational features utilised to study the dynamic nature of the Galaxy's spiral structure. With the most updated samples of high-mass star formation region (HMSFR) masers, O stars and open clusters, we investigated their distributions and kinematic properties in the vicinity of the Sun. We fo…

2021 Research in Astronomy and Astrophysics
Gaia 7
Serendipitous discovery of a dusty disc around WDJ181417.84-735459.83
DOI: 10.1093/mnras/staa3836 Bibcode: 2021MNRAS.501.3916G

Cooper, W. J.; Marocco, F.; Koester, D. +8 more

Spectroscopic observations of white dwarfs reveal that many of them are polluted by exoplanetary material, whose bulk composition can be uniquely probed this way. We present a spectroscopic and photometric analysis of the DA white dwarf WDJ181417.84-735459.83, an object originally identified to have a strong infrared (IR) excess in the 2MASS and W…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 7
Modeling Stellar Abundance Patterns Resulting from the Addition of Earth-like Planetary Material
DOI: 10.3847/1538-3881/abdf5d Bibcode: 2021AJ....161..142C

Cowley, Charles R.; Bord, Donald J.; Yüce, Kutluay

We model the observed precision differential abundance patterns of three G-type dwarfs, assuming a mass of planetary or disk material was added to or subtracted from the atmosphere of the star. The two-parameter model is fit by linear regression. The stellar abundance patterns are corrected for Galactic chemical evolution (GCE). The differential a…

2021 The Astronomical Journal
Hipparcos 7
Detection of volatiles undergoing sublimation from 67P/Churyumov-Gerasimenko coma particles using ROSINA/COPS. I. The ram gauge
DOI: 10.1051/0004-6361/202039130 Bibcode: 2021A&A...645A..38P

Altwegg, K.; Balsiger, H.; Rubin, M. +5 more

Context. The ESA Rosetta mission has allowed for an extensive in situ study of the comet 67P/Churyumov-Gerasimenko. In measurements performed by the ram gauge of the COmet Pressure Sensor (COPS), observed features are seen to deviate from the nominal ram gauge signal. This effect is attributable to the sublimation of the volatile fraction of comet…

2021 Astronomy and Astrophysics
Rosetta 7
uGMRT detection of cluster radio emission in low-mass Planck Sunyaev-Zel'dovich clusters
DOI: 10.1093/mnras/stab1965 Bibcode: 2021MNRAS.506.5389P

Raychaudhury, Somak; Paul, Surajit; Dabhade, Pratik +5 more

Low-mass (M500 < 5 × 1014 M) galaxy clusters have been largely unexplored in radio observations, because of the inadequate sensitivity of existing telescopes. However, the upgraded Giant Metrewave Radio Telescope (uGMRT) and the Low Frequency ARray (LoFAR), with unprecedented sensitivity at low frequencies, hav…

2021 Monthly Notices of the Royal Astronomical Society
XMM-Newton 7
The role of magnetospheric plasma in solar wind-magnetosphere coupling: A review
DOI: 10.1016/j.jastp.2021.105644 Bibcode: 2021JASTP.21905644W

Walsh, Brian M.; Zou, Ying

A variety of magnetospheric plasma populations have been proposed to impact solar wind-magnetosphere coupling. These magnetospheric populations could mass load the dayside magnetopause and include the plasmaspheric plume, plasma cloak, ion plasma sheet, and dayside ion outflow. Each has different densities, ion composition, and spatial/temporal oc…

2021 Journal of Atmospheric and Solar-Terrestrial Physics
Cluster 7