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Milky Way-like galaxies: stellar population properties of dynamically defined discs, bulges and stellar haloes
DOI: 10.1093/mnras/stac2033 Bibcode: 2022MNRAS.516..197O

Tissera, Patricia B.; Obreja, Aura; Ortega-Martinez, Sara +3 more

The formation of galaxies can be understood in terms of the assembly patterns of each type of galactic component. To perform this kind of analysis, it is necessary to define some criteria to separate those components. Decomposition methods based on dynamical properties are more physically motivated than photometry-based ones. We use the unsupervis…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 7
The HDO Cycle on Mars: Comparison of ACS Observations With GCM Simulations
DOI: 10.1029/2022JE007201 Bibcode: 2022JGRE..12707201R

Montmessin, Franck; Trokhimovskiy, Alexander; Alday, Juan +10 more

The D/H ratio and its implications on the atmospheric escape, make it an essential observable to study the current and past inventory of water on Mars. With the arrival of the Trace Gas Orbiter around Mars, new measurements of the D/H ratio are now available and require tools to interpret the observations and understand the HDO cycle. We here pres…

2022 Journal of Geophysical Research (Planets)
ExoMars-16 7
Optical Observations of the Nearby Type Ia Supernova 2021hpr
DOI: 10.1088/1538-3873/ac7583 Bibcode: 2022PASP..134g4201Z

Zhang, Yu; Zhang, Tianmeng; Wu, Hong +6 more

We present the optical photometric and spectroscopic observations of the nearby Type Ia supernova (SN) 2021hpr. The observations covered the phase of -14.37 to +63.68 days relative to its maximum luminosity in the B band. The evolution of multiband light/color curves of SN 2021hpr is similar to that of normal Type Ia supernovae (SNe Ia) with the e…

2022 Publications of the Astronomical Society of the Pacific
eHST 7
SWIFT J0503.7-2819: a nearly synchronous intermediate polar below the period gap?
DOI: 10.1093/mnras/stac2723 Bibcode: 2022MNRAS.517.1667R

Pandey, J. C.; Scaringi, Simone; Joshi, Arti +2 more

Based on the X-ray observations from XMM-Newton and Swift, and optical observations from Transiting Exoplanet Survey Satellite (TESS) and AAVSO, we present temporal and spectral properties of probable intermediate polar SWIFT J0503.7-2819. The X-ray light curve shows two distinctive features, where possibly the second pole seems to be active durin…

2022 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 7
Young, Blue, and Isolated Stellar Systems in the Virgo Cluster. II. A New Class of Stellar System
DOI: 10.3847/1538-4357/ac7c6c Bibcode: 2022ApJ...935...51J

Cresci, Giovanni; Cannon, John M.; Haynes, Martha P. +21 more

We discuss five blue stellar systems in the direction of the Virgo cluster, analogous to the enigmatic object SECCO 1 (AGC 226067). These objects were identified based on their optical and UV morphology and followed up with H I observations with the Very Large Array (and Green Bank Telescope), Multi Unit Spectroscopic Explorer (on the Very Large T…

2022 The Astrophysical Journal
eHST 7
Searching for nascent planetary nebulae: OHPNe candidates in the SPLASH survey
DOI: 10.1093/mnras/stac2341 Bibcode: 2022MNRAS.516.2235C

Miranda, Luis F.; de Gregorio-Monsalvo, Itziar; Imai, Hiroshi +7 more

The evolution of asymptotic giant branch stars from the spherical symmetry into the diverse shapes of planetary nebulae (PNe) is a topic of intensive research. Young PNe provide a unique opportunity to characterize the onset of this transitional phase. In particular, OH maser-emitting PNe (OHPNe) are considered nascent PNe. In fact, only six OHPNe…

2022 Monthly Notices of the Royal Astronomical Society
AKARI Gaia Herschel 7
A comprehensive photometric and kinematical characteristic of the newly discovered QCs clusters with Gaia EDR3
DOI: 10.1007/s12036-022-09810-1 Bibcode: 2022JApA...43...26E

Elsanhoury, W. H.; Haroon, A. A.; Amin, Magdy Y. +1 more

This study reports the first comprehensive astrometric, photometric, and kinematical analysis of four newly discovered open clusters; namely QC1, QC2, QC3, and QC4, using astrometric and photometric data from the most recent Gaia EDR3 for G<17

2022 Journal of Astrophysics and Astronomy
Gaia 7
QU Vul: An integral field spectroscopy case study of a nova shell
DOI: 10.1093/mnras/stac2789 Bibcode: 2022MNRAS.517.2567S

Guerrero, M. A.; Toalá, J. A.; Santamaría, E. +2 more

We present GTC MEGARA high-dispersion integral field spectroscopic observations of the nova remnant QU Vul, which provide a comprehensive 3D view of this nova shell. The tomographic analysis of the H α emission reveals a complex physical structure characterized by an inhomogeneous and clumpy distribution of the material within this shell. The over…

2022 Monthly Notices of the Royal Astronomical Society
Gaia eHST 7
New Results from the Spectral Observations of Solar Coronal Type II Radio Bursts
DOI: 10.3847/1538-4357/ac4bd6 Bibcode: 2022ApJ...926...38R

Ramesh, R.; Kathiravan, C.; Natarajan, S. Surya

We carried out a statistical study of twenty-six type II radio bursts from the Sun observed with the Gauribidanur Low-frequency Solar Spectrograph in the frequency range 85-35 MHz during the period 2009-2019. Our results indicate that the average instantaneous bandwidth of the type II bursts in the above frequency range correlates with the angular…

2022 The Astrophysical Journal
SOHO 7
Broadband X-Ray Spectral Analysis of the Dual AGN System Mrk 739
DOI: 10.3847/1538-4357/ac97ec Bibcode: 2022ApJ...939...88I

Tanimoto, Atsushi; Ueda, Yoshihiro; Ricci, Claudio +4 more

We present the result of a broadband (0.5-70 keV) X-ray spectral analysis of the late-merger galaxy Mrk 739, which contains a dual active galactic nucleus (AGN), Mrk 739E and Mrk 739W, with a separation of ≈3.4 kpc. The spectra obtained with NuSTAR, Chandra, XMM-Newton, and Swift/BAT are simultaneously analyzed by separating the contributions from…

2022 The Astrophysical Journal
XMM-Newton 7