Search Publications

Influence of the Gaia-Sausage-Enceladus on the Density Shape of the Galactic Stellar Halo Revealed by Halo K Giants from the LAMOST Survey
DOI: 10.3847/1538-3881/ac746e Bibcode: 2022AJ....164...41W

Zhao, Gang; Yang, Chengqun; Pei, Wenxiang +2 more

We present a study of the influence of the Gaia-Sausage-Enceladus (GSE) on the density shape of the Galactic stellar halo using 11,624 K giants from the LAMOST survey. Every star is assigned a probability of being a member of the GSE based on its spherical velocities and metallicity by a Gaussian mixture model. We divide the stellar halo into two …

2022 The Astronomical Journal
Gaia 11
UV and X-ray pulse amplitude variability in the transitional millisecond pulsar PSR J1023+0038
DOI: 10.1051/0004-6361/202243180 Bibcode: 2022A&A...660A..63M

D'Avanzo, P.; Campana, S.; Stella, L. +7 more

The transitional millisecond pulsar PSR J1023+0038 is the first millisecond pulsar discovered to emit UV and optical pulses. Here we present the results of the UV and X-ray phase-resolved timing analysis of observations performed with the Hubble Space Telescope, XMM-Newton, and NuSTAR satellites between 2014 and 2021. Ultraviolet pulsations are de…

2022 Astronomy and Astrophysics
XMM-Newton eHST 11
Concordance between Observations and Simulations in the Evolution of the Mass Relation between Supermassive Black Holes and Their Host Galaxies
DOI: 10.3847/1538-4357/ac714c Bibcode: 2022ApJ...933..132D

Treu, Tommaso; Bhowmick, Aklant K.; Blecha, Laura +7 more

We carry out a comparative analysis of the relation between the mass of supermassive black holes (BHs) and the stellar mass of their host galaxies at 0.2 < z < 1.7 using well-matched observations and multiple state-of-the-art simulations (e.g., MassiveBlackII, Horizon-AGN, Illustris, TNG, and a semianalytic model). The observed sample consis…

2022 The Astrophysical Journal
eHST 11
Searching for Compact Objects in Binaries with Gaia DR3
DOI: 10.3847/1538-4357/ac9b4c Bibcode: 2022ApJ...940..126F

Liu, Jifeng; Gu, Wei-Min; Yi, Tuan +4 more

We search for compact objects in binaries based on Gaia DR3. A sample of 10 targets is derived under the following conditions: the radial velocity variable, low temperature (T eff < 6000 K), high mass function (f(M 2) > 1M ), and ellipsoidal-like light curves. Two targets have LAMOST spectroscopic observatio…

2022 The Astrophysical Journal
Gaia 11
Multiwavelength properties of 850-µm selected sources from the North Ecliptic Pole SCUBA-2 survey
DOI: 10.1093/mnras/stac1105 Bibcode: 2022MNRAS.514.2915S

Goto, Tomotsugu; Kim, Seong Jin; Conselice, Christopher J. +25 more

We present the multiwavelength counterparts of 850-$\mu$m selected submillimetre sources over a 2-deg2 field centred on the North Ecliptic Pole. In order to overcome the large beam size (15 arcsec) of the 850-$\mu$m images, deep optical to near-infrared (NIR) photometric data and arcsecond-resolution 20-cm images are used to identify co…

2022 Monthly Notices of the Royal Astronomical Society
AKARI Herschel 11
Synthetic solar cycle for active regions violating the Hale's polarity law
DOI: 10.1093/mnras/stac597 Bibcode: 2022MNRAS.512.1365Z

Abramenko, V.; Sokoloff, D.; Zhukova, A. +1 more

Long observational series for bipolar active regions (ARs) provide significant information about the mutual transformation of the poloidal and toroidal components of the global solar magnetic field. The direction of the toroidal field determines the polarity of leading sunspots in ARs in accordance with the Hale's polarity law. The vast majority o…

2022 Monthly Notices of the Royal Astronomical Society
SOHO 11
The MURALES survey. VI. Properties and origin of the extended line emission structures in radio galaxies
DOI: 10.1051/0004-6361/202142823 Bibcode: 2022A&A...662A..23B

Marconi, A.; Capetti, A.; Gilli, R. +11 more

This is the sixth paper presenting the results of the MUse RAdio Loud Emission line Snapshot survey. We observed 37 radio sources from the 3C sample with z < 0.3 and a declination < 20° with the Multi Unit Spectroscopic Explorer optical integral field spectrograph at the Very Large Telescope. Here, we focus on the properties of the extended …

2022 Astronomy and Astrophysics
eHST 11
Apparent Motion of the Circumstellar Envelope of CQ Tau in Scattered Light
DOI: 10.3847/1538-3881/ac36cb Bibcode: 2022AJ....163...31S

Strakhov, Ivan A.; Goliguzova, Maria V.; Safonov, Boris S. +1 more

The study of spiral structures in protoplanetary disks is of great importance for understanding the processes in the disks, including planet formation. Bright spiral arms were detected in the disk of young star CQ Tau by Uyama et al. in the H and L bands. The spiral arms are located inside the gap in millimeter-sized dust, discovered earlier using…

2022 The Astronomical Journal
Gaia 11
The detection of radio emission from known X-ray flaring star EXO 040830-7134.7
DOI: 10.1093/mnras/stab3461 Bibcode: 2022MNRAS.510.1083D

Woudt, P. A.; Williams, D. R. A.; Fender, R. P. +4 more

We report the detection of radio emission from the known X-ray flaring star EXO 040830-7134.7 during Karoo Array Telescope (MeerKAT) observations of the nearby cataclysmic variable VW Hydri. We have three epochs of MeerKAT observations, where the star is not detected in the first epoch, is detected in the second epoch, and is marginally detected i…

2022 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 11
Evidence for a milliparsec-separation supermassive binary black hole with quasar microlensing
DOI: 10.1051/0004-6361/202244440 Bibcode: 2022A&A...668A..77M

Courbin, F.; Sluse, D.; Lemon, C. +4 more

We report periodic oscillations in the 15-year-long optical light curve of the gravitationally lensed quasar Q J0158−4325 at zs = 1.29. The signal is enhanced during a high magnification microlensing event of the quasar that the fainter lensed image, B, underwent between 2003 and 2010. We measure a period of Po = 172.6 ± 0.9 …

2022 Astronomy and Astrophysics
eHST 11