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Gaia DR2 and EDR3 data and evolutionary status of post-AGB stars with high radial velocities
DOI: 10.1093/pasj/psac074 Bibcode: 2022PASJ...74.1368A

Matsuno, Tadafumi; Aoki, Wako; Parthasarathy, Mudumba

Using the Gaia Data Release 2 (DR2) and Early Data Release 3 (EDR3) data and list of post-AGB candidates, we investigate the parallax, proper motion, and binarity for 20 post-AGB stars and candidates that have high radial velocities. From their Gaia distances, their luminosities and kinematics are derived. The evolutionary status of these stars is…

2022 Publications of the Astronomical Society of Japan
Gaia 2
The Small Separation A-star Companion Population: First Results with CHARA/MIRC-X
DOI: 10.3847/1538-4357/aca1ad Bibcode: 2022ApJ...941..118D

Lanthermann, Cyprien; Anugu, Narsireddy; Kraus, Stefan +9 more

We present preliminary results from our long-baseline interferometry (LBI) survey to constrain the multiplicity properties of intermediate-mass A-type stars within 80 pc. Previous multiplicity studies of nearby stars exhibit orbital separation distributions well fitted with a lognormal with peaks >15 au, increasing with primary mass. The A-star…

2022 The Astrophysical Journal
Gaia 2
Identification and Parameter Determination of F-type Herbig Stars from LAMOST DR8
DOI: 10.3847/1538-4357/ac84da Bibcode: 2022ApJ...936..151Z

Luo, A. -Li; Hou, Wen; Jiang, Biwei +5 more

We identify 20 F-type Herbig stars and provide a list of 22 pre-main-sequence candidates from LAMOST DR8. The effective temperature, distance, extinction, stellar luminosity, mass, age, and radius are derived for each Herbig star based on optical spectra, photometry, Gaia EDR3 parallaxes, and pre-main-sequence evolutionary tracks. According to spe…

2022 The Astrophysical Journal
AKARI Gaia 2
Evolved eclipsing binary systems in the Galactic bulge: Precise physical and orbital parameters of OGLE-BLG-ECL-305487 and OGLE-BLG-ECL-116218
DOI: 10.1051/0004-6361/202244433 Bibcode: 2022A&A...668A..30S

Smolec, R.; Thompson, I. B.; Villanova, S. +17 more


Aims: Our goal is to determine, with high accuracy, the physical and orbital parameters of two double-lined eclipsing binary systems, where the components are two giant stars. We also aim to study the evolutionary status of the binaries, to derive the distances towards them by using a surface brightness-colour relation, and to compare these m…

2022 Astronomy and Astrophysics
Gaia 2
CORALIE radial velocity search for companions around evolved stars (CASCADES). II. Seismic masses for three red giants orbited by long-period massive planets
DOI: 10.1051/0004-6361/202040079 Bibcode: 2022A&A...657A..88B

Buldgen, G.; Eggenberger, P.; Ségransan, D. +10 more

Context. The advent of asteroseismology as the golden path to precisely characterize single stars naturally led to synergies with the field of exoplanetology. Today, the precise determination of stellar masses, radii and ages for exoplanet-host stars is a driving force in the development of dedicated software and techniques to achieve this goal. H…

2022 Astronomy and Astrophysics
Gaia 2
Development of Chaos Terrain as Subaqueous Slide Blocks in Galilaei Crater, Mars
DOI: 10.3390/rs14091998 Bibcode: 2022RemS...14.1998N

Nizam, Nabila; Divola, Claire; Day, Mackenzie +2 more

Chaos terrain, expressed as enigmatic blocky landscapes on Mars, has poorly understood origins. Several hypotheses have been put forward to explain chaos terrain formation, but none fully account for the morphologies observed in Galilaei crater, the focus of this study. Previously inferred to be a paleolake, Galilaei crater hosts chaos terrain com…

2022 Remote Sensing
MEx 2
The evolutionary state of the chemically peculiar members of the open cluster NGC 2516
DOI: 10.1093/mnras/stac1769 Bibcode: 2022MNRAS.515.3094K

Hubrig, S.; Schöller, M.; Piskunov, A. E. +1 more

We aim at establishing safe membership and evolutionary status of 11 chemically peculiar (CP) stars that are residing in the domain of the open cluster NGC 2516 and are frequently referred to as cluster members. We queried the Gaia EDR3 catalogue in an area with a radius of 1° and selected 37 508 stars brighter than G = 19 mag. The cluster members…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 2
Improving Multiday Solar Wind Speed Forecasts
DOI: 10.1029/2021SW002868 Bibcode: 2022SpWea..2002868E

Arge, C. N.; Henney, C. J.; Dayeh, M. A. +4 more

We analyze the residual errors for the Wang-Sheeley-Arge (WSA) solar wind speed forecasts as a function of the photospheric magnetic field expansion factor (fp) and the minimum separation angle (d) in the photosphere between the footpoints of open field lines and the nearest coronal hole boundary. We find the map of residual speed error…

2022 Space Weather
Ulysses 2
C,T1,T2: A Complementary Method to Detect Multiple Populations with the Washington Filter System
DOI: 10.22201/ia.01851101p.2022.58.02.02 Bibcode: 2022RMxAA..58..181F

Geisler, D.; Villanova, S.; Frelijj, H. +1 more

In this research we test the ability of a three Washington filter combination, (C − T1) − (T1 − T2), compared with that of the traditional C − T1 color to find multiple populations on two globular clusters: NGC 7099 and NGC 1851, types I and II Globular clusters, respectively. Our improved photometry and…

2022 Revista Mexicana de Astronomia y Astrofisica
Gaia eHST 2
XMM-Newton detection of soft time lags in the TDE candidate AT 2018fyk
DOI: 10.1093/mnrasl/slab133 Bibcode: 2022MNRAS.511L..19Z

Zhang, Wenda

In this letter, we report a tentative detection of soft time lags (i.e. variability of softer photons lags behind the variability of harder photons) in one XMM-Newton observation of the tidal disruption event (TDE) candidate AT 2018fyk while the source was in the hard spectral state. The lags are detected at $6.51\times 10^{-5}~\rm Hz$. The amplit…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 2