Search Publications

First photometric investigation of two short-period eclipsing binaries ASAS J105115-6032.1 and GDS J1056047-604149
DOI: 10.1016/j.newast.2021.101756 Bibcode: 2022NewA...9301756L

Sarotsakulchai, Thawicharat; Soonthornthum, Boonrucksar; Liu, Nian-Ping +1 more

ASAS J105115-6032.1 (hereafter ASAS J1051) and GDS J1056047-604149 (hereafter GDS J1056) are two short-period contact binaries close to each other in the Antarctica sky area. By analyzing the light curves from AST3-1, the first photometric solutions are presented using the Wilson-Devinney (W-D) method. It is detected that both systems are W-type c…

2022 New Astronomy
Gaia 2
Hot white dwarf candidates from the IGAPS-GALEX cross-match
DOI: 10.1093/mnras/stac1403 Bibcode: 2022MNRAS.514.2434G

Raddi, R.; Sabin, L.; Gómez-Muñoz, M. A. +1 more

White dwarf (WD) stars are often associated with the central stars of planetary nebulae (CSPNe) on their way to the cooling track. A large number of WD star candidates have been identified; thanks to optical large-scale surveys such as Gaia DR2 and EDR3. However, hot-WD/CSPNe stars are quite elusive in optical bands due to their high temperatures …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 2
Abundances of disk and bulge giants from high-resolution optical spectra. V. Molybdenum: The p-process element
DOI: 10.1051/0004-6361/202244013 Bibcode: 2022A&A...666A.125F

Ryde, N.; Rich, R. M.; Jönsson, H. +2 more


Aims: In this work, we aim to make a differential comparison of the neutron-capture and p-process element molybdenum (Mo) in the stellar populations in the local disk(s) and the bulge, focusing on minimising possible systematic effects in the analysis.
Methods: The stellar sample consists of 45 bulge and 291 local disk K-giants observed …

2022 Astronomy and Astrophysics
Gaia 2
Simulation of Water Vapor Photodissociation during Dust Storm Season on Mars
DOI: 10.1134/S0038094622010051 Bibcode: 2022SoSyR..56...23S

Medvedev, A. S.; Rodin, A. V.; Shaposhnikov, D. S.

Within the framework of this work, using a three-dimensional numerical model of the general circulation of the Martian atmosphere MAOAM (Martian Atmosphere: Observation and Modeling), also known as MPI-MGCM (Max Planck Institute Martian General Circulation Model), we simulated the planet's hydrological cycle during the 28 and 34 Martian years (MY2…

2022 Solar System Research
ExoMars-16 2
Improvements to Pan-STARRS1 Astrometry. II. Corrections for Differential Chromatic Refraction
DOI: 10.3847/1538-3881/ac7ab6 Bibcode: 2022AJ....164...73W

White, Richard L.; Shiao, Bernie; Lubow, Stephen H.

In a previous paper, we applied the Gaia DR2 catalog to improve the astrometric accuracy of about 1.7 billion objects in Pan-STARRS1 Data Release 2 (PS1 DR2). We report here on further improvements made by utilizing Gaia EDR3 and correcting for the effects of differential chromatic refraction (DCR) in decl. We extend the correction algorithm in Pa…

2022 The Astronomical Journal
Gaia 2
Detection of a Superluminous Spiral Galaxy in the Heart of a Massive Galaxy Cluster
DOI: 10.3847/1538-4357/ac62cd Bibcode: 2022ApJ...930..138B

Lovisari, Lorenzo; Ogle, Patrick; Jones, Christine +5 more

It is well established that brightest cluster galaxies (BCGs), residing in the centers of galaxy clusters, are typically massive and quenched galaxies with cD or elliptical morphology. An optical survey suggested that an exotic galaxy population, superluminous spiral and lenticular galaxies, could be the BCGs of some galaxy clusters. Because the c…

2022 The Astrophysical Journal
XMM-Newton 2
Suzaku observations of Fe K-shell lines in the supernova remnant W 51 C and hard X-ray sources in the proximity
DOI: 10.1093/pasj/psac026 Bibcode: 2022PASJ...74..656S

Fujita, Yutaka; Nobukawa, Masayoshi; Nobukawa, Kumiko K. +2 more

In this paper, we investigate the Fe K-shell lines in the supernova remnant W 51 C and hard X-ray sources in the proximity. We measure the intensities of the Fe I Kα and Fe XXV Heα lines at 6.40 and 6.68 keV, respectively, and find that the intensity of the 6.68 keV line is consistent with the background level expected from previous studies, while…

2022 Publications of the Astronomical Society of Japan
Suzaku 2
Recent Formation of a Spiral Disk Hosting Progenitor Globular Clusters at the Center of the Perseus Brightest Cluster Galaxy. I. Spiral Disk
DOI: 10.3847/1538-4357/ac4df5 Bibcode: 2022ApJ...927..137Y

Ohyama, Youichi; Lim, Jeremy; Yeung, Michael C. H.

We address the nature and origin of a spiral disk at the center of NGC 1275, the giant elliptical galaxy at the center of the Perseus cluster, that spans a radius of ~5 kpc. By comparing stellar absorption lines measured in long-slit optical spectra with synthetic spectra for single stellar populations, we find that fitting of these lines requires…

2022 The Astrophysical Journal
eHST 2
An investigation into the spectral parameters of ultra-low-frequency (ULF) waves in the polar caps and magnetotail
DOI: 10.5194/angeo-40-151-2022 Bibcode: 2022AnGeo..40..151N

Nosikova, Nataliya Sergeevna; Yagova, Nadezda Viktorovna; Baddeley, Lisa Jane +2 more

The present case study is focused on fluctuations at ∼ 1.5 mHz observed on open field lines in both of the polar caps in ground-based geomagnetic data and in the electron concentration in the Northern Hemisphere ionosphere. Coherent pulsations with a relatively narrow narrowband-like spectra and a higher fraction of transversal components in the t…

2022 Annales Geophysicae
Cluster 2
Estimation of the Mass of the Very Massive Galaxy Cluster SRGe CL2305.2-2248 from Strong Lensing
DOI: 10.1134/S1063773722010042 Bibcode: 2022AstL...48....1K

Bikmaev, I. F.; Gilfanov, M. R.; Khamitov, I. M. +10 more

SRGe CL2305.2-2248 (SPT-CL J2305-2248, ACT-CL J2305.1-2248) is one of the most massive galaxy clusters at high redshifts ($z∼eq 0.76$) and is of great interest for cosmology. Deep images have been obtained at the Russian-Turkish 1.5-m telescope (RTT-150) for an optical identification of this cluster. In combination with the open Hubble Space Teles…

2022 Astronomy Letters
eHST 2