Search Publications

Investigating dynamical properties of globular clusters through a family of lowered isothermal models
DOI: 10.1093/mnras/stac3520 Bibcode: 2023MNRAS.519..445C

Jiang, Ing-Guey; Cheng, Chia-Hsuan

To investigate the dynamical properties of globular clusters, surface brightness and kinematic data were collected and fitted to a family of lowered isothermal models called LIMEPY models. For the 18 globular clusters studied, the amounts of concentration, truncation, and anisotropy were determined. In addition, the cluster mass, half-mass radius,…

2023 Monthly Notices of the Royal Astronomical Society
Gaia eHST 2
The formation of cone chains in the Chryse Planitia region on Mars and the thermodynamic aspects of this process
DOI: 10.1016/j.icarus.2023.115473 Bibcode: 2023Icar..39615473C

Czechowski, Leszek; Zalewska, Natalia; Zambrowska, Anita +3 more

This paper considers a small region in Chryse Planitia where several subparallel chains of cones are observed. Despite many papers on small Martian cones, the mechanism of their formation is not unequivocally explained, nor the reason for their arrangement in subparallel chains. In this paper, we test a few hypotheses stating that most of the cone…

2023 Icarus
MEx 2
Gaia DR3 and nearby galaxies: where do foregrounds matter?
DOI: 10.1093/mnras/stac3289 Bibcode: 2023MNRAS.518.3746B

Barmby, P.

Nearby galaxies provide populations of stellar and non-stellar sources at a common distance and in quantifiable environments. All are observed through the Milky Way foreground, with varying degrees of contamination that depend on observed Galactic latitude and the distance and size of the target galaxy. This work uses Gaia Data Release 3 (DR3) to …

2023 Monthly Notices of the Royal Astronomical Society
Gaia 2
A Machine Learning Enhanced Approach for Automated Sunquake Detection in Acoustic Emission Maps
DOI: 10.1007/s11207-022-02081-7 Bibcode: 2023SoPh..298....4M

Besliu-Ionescu, Diana; Mercea, Vanessa; Paraschiv, Alin Razvan +2 more

Sunquakes are seismic emissions visible on the solar surface, associated with some solar flares. Although discovered in 1998, they have only recently become a more commonly detected phenomenon. Despite the availability of several manual detection guidelines, to our knowledge, the astrophysical data produced for sunquakes is new to the field of mac…

2023 Solar Physics
SOHO 2
A closer look at NGC 7314 nuclear region: a multiwavelength analysis of the Seyfert nucleus and its surroundings
DOI: 10.1093/mnras/stac3454 Bibcode: 2023MNRAS.519.1293D

Arévalo, P.; López-Navas, E.; Menezes, R. B. +4 more

The central regions of galaxies harbouring active galactic nuclei (AGNs) can be quite complex, especially at high activity, presenting, besides variability, a variety of phenomena related, e.g. to ionization/excitation mechanisms. A detailed study is necessary in order to understand better those objects. For that reason, we performed a multiwavele…

2023 Monthly Notices of the Royal Astronomical Society
XMM-Newton eHST 2
Investigating the vertical distribution of the disk as a function of radial action
DOI: 10.1051/0004-6361/202142977 Bibcode: 2023A&A...669A.107J

Zhao, Gang; Chen, Yuqin; Du, Cuihua +1 more


Aims: As heating processes can broaden the distributions of radial actions and the vertical distributions of the Galactic disks, we investigate the vertical distribution of the Galactic disks as a function of radial action based on Apache Point Observatory Galactic Evolution Experiment (APOGEE) and Gaia data in order to deepen our understandi…

2023 Astronomy and Astrophysics
Gaia 2
In the Trenches of the Solar-Stellar Connection. VII. Wilson-Bappu 2022
DOI: 10.3847/1538-4365/acb535 Bibcode: 2023ApJS..266....6A

Ayres, Thomas

The Wilson-Bappu effect (WBE) is a remarkable correlation between the width of the chromospheric emission core of the Ca II 3934 Å K line and stellar absolute visual magnitude over an astonishing range, from diminutive red dwarfs to bloated yellow supergiants. The WBE signifies a deep connection between the nonclassical, mechanically heated chromo…

2023 The Astrophysical Journal Supplement Series
Gaia IRIS IUE eHST 2
Small-Scale Upflows in a Coronal Hole - Tracked from the Photosphere to the Corona
DOI: 10.1007/s11207-023-02216-4 Bibcode: 2023SoPh..298..129S

Barczynski, Krzysztof; Orozco Suárez, David; Mandrini, Cristina H. +4 more

Coronal transients are known as sources of coronal upflows. With the commissioning of Solar Orbiter, it became apparent that coronal small-scale features are even more frequent than previously estimated. It was found that even small coronal features seen by Solar Orbiter can produce visible upflows. Therefore, it is important to study the plasma f…

2023 Solar Physics
Hinode IRIS SolarOrbiter 2
Validation of TOI-1221 b: A Warm Sub-Neptune Exhibiting Transit Timing Variations around a Sun-like Star
DOI: 10.3847/1538-3881/acc8d4 Bibcode: 2023AJ....165..217M

Kristiansen, Martti H.; Torres, Guillermo; Hellier, Coel +25 more

We present a validation of a long-period ( ${91.68278}_{-0.00041}^{+0.00032}$ days) transiting sub-Neptune planet, TOI-1221 b (TIC 349095149.01), around a Sun-like (m V = 10.5) star. This is one of the few known exoplanets with a period >50 days, and belongs to the even smaller subset of which have bright enough hosts for detailed …

2023 The Astronomical Journal
Gaia 2
Are Nonthermal Velocities in Active Region Coronal Loops Anisotropic?
DOI: 10.3847/1538-4357/acdfd2 Bibcode: 2023ApJ...953....3H

Hahn, Michael; Asgari-Targhi, Mahboubeh; Savin, Daniel Wolf

We have measured line widths in active region coronal loops in order to determine whether the nonthermal broadening is anisotropic with respect to the magnetic field direction. These nonthermal velocities are caused by unresolved fluid motions. Our analysis method combines spectroscopic data and a magnetic field extrapolation. We analyzed spectra …

2023 The Astrophysical Journal
Hinode 2