Search Publications

Test for Echo: X-Ray Reflection Variability in the Seyfert-2 Active Galactic Nucleus NGC 4388
DOI: 10.3847/1538-4357/ad2fa3 Bibcode: 2024ApJ...966...57G

Brandt, W. N.; Arzoumanian, Zaven; Gendreau, Keith +4 more

We report on a study of the narrow Fe Kα line and reflection spectrum in the well-known Seyfert-2 active galactic nucleus (AGN), NGC 4388. X-ray spectra summed from two extensive NICER monitoring campaigns, separated by years, show strong evidence of variation in the direct continuum and reflected emission, but only small variations in the obscuri…

2024 The Astrophysical Journal
INTEGRAL 0
X-ray Observations of the Intermediate Polar TX Col
DOI: 10.25518/0037-9565.11662 Bibcode: 2024BSRSL..93..243P

Joshi, Arti; Rawat, Nikita; Rao, Srinivas M. +2 more

We present the timing analysis of the intermediate polar TX Col in the X-ray band using the observations made by Chandra, Swift, and Suzaku during the years 2000, 2007, and 2009, respectively. The spin, orbital, and beat periods derived from these data are consistent with the earlier findings. We found that the spin modulation was dominant during …

2024 Bulletin de la Societe Royale des Sciences de Liege
Gaia Suzaku 0
Se-ResNet+SVM Model: An Effective Method of Searching for Hot Subdwarfs from LAMOST
DOI: 10.3847/1538-4365/ad5b61 Bibcode: 2024ApJS..274....2C

Wu, Tianmin; Yi, Zhenping; Lei, Zhenxin +7 more

This paper presents a robust neural network approach for identifying hot subdwarfs. Our method leveraged the Squeeze-and-Excitation Residual Network to extract abstract features, which were combined with experience features to create hybrid features. These hybrid features were then classified using a support vector machine. To enhance accuracy, we…

2024 The Astrophysical Journal Supplement Series
Gaia 0
V0405 Dra: A New Deep and Low Mass Ratio Contact Binary with Extremely Fast Decrease in the Orbital Period
DOI: 10.1088/1674-4527/ad47dd Bibcode: 2024RAA....24f5023L

Zheng, Jie; Jiang, Lin-Qiao; Tian, Xiao-Man +5 more

V0405 Dra is a W UMa-type binary star. Based on the TESS data, we have conducted an orbital period study and performed a light curve analysis for the system. The orbital period study reveals that the O ‑ C curve for V0405 Dra exhibits secular decrease at an extremely high rate of dP/dt = ‑2.71 × 10‑6 day year‑1, along with pe…

2024 Research in Astronomy and Astrophysics
Gaia 0
Searching for new cataclysmic variables in different X-ray and optical catalogs
DOI: 10.51194/INASAN.2024.9.3.007 Bibcode: 2024INASR...9..118G

Galiullin, I. I.

Cataclysmic variables (CVs) are binary systems in which a white dwarf accretes matter from a Roche-lobe-filling companion star. Numerous CVs can be seen in optical light curves as periodic sources. Moreover, accretion can result in outbursts, which are visible in their optical light curves, especially in non-magnetic CVs. I review a modern multiwa…

2024 INASAN Science Reports
Gaia 0
MUSE-ALMA Haloes X: the stellar masses of gas-rich absorbing galaxies
DOI: 10.1093/mnras/stae387 Bibcode: 2024MNRAS.528.6159A

Hayes, M.; Kacprzak, G. G.; Kuntschner, H. +13 more

The physical processes by which gas is accreted onto galaxies, transformed into stars, and then expelled from galaxies are of paramount importance to galaxy evolution studies. Observationally constraining each of these baryonic components in the same system, however, is challenging. Furthermore, simulations indicate that the stellar mass of galaxi…

2024 Monthly Notices of the Royal Astronomical Society
eHST 0
Temperature anisotropy instabilities driven by intermittent velocity shears in the solar wind
DOI: 10.1017/S0022377824001375 Bibcode: 2024JPlPh..90f9002O

Sorriso-Valvo, Luca; Verscharen, Daniel; Chen, Christopher H. K. +5 more

Where and under what conditions the transfer of energy between electromagnetic fields and particles takes place in the solar wind remains an open question. We investigate the conditions that promote the growth of kinetic instabilities predicted by linear theory to infer how turbulence and temperature-anisotropy-driven instabilities are interrelate…

2024 Journal of Plasma Physics
SolarOrbiter 0
Reconstructing the mid-infrared spectra of galaxies using ultraviolet to submillimeter photometry and Deep Generative Networks
DOI: 10.1016/j.ascom.2024.100823 Bibcode: 2024A&C....4700823R

Efstathiou, A.; Rissaki, Agapi; Pavlou, O. +2 more

The mid-infrared spectra of galaxies are rich in features such as the Polycyclic Aromatic Hydrocarbon (PAH) and silicate dust features which give valuable information about the physics of galaxies and their evolution. For example they can provide information about the relative contribution of star formation and accretion from a supermassive black …

2024 Astronomy and Computing
Herschel 0
A summary of instruments proposed for observing pulsating variables from the Mt. Abu Observatory
DOI: 10.1007/s12036-024-10019-7 Bibcode: 2024JApA...45...34M

Ganesh, Shashikiran; Prajapati, Prachi; Mishra, Anwesh Kumar +3 more

Pulsating variables play a significant role in shaping modern astronomy. Presently it is an exciting era in observational study of variable stars owing to surveys like OGLE and TESS. The vast number of sources being discovered by these surveys is also creating opportunities for 1–2-m class telescopes to provide follow-up observations to characteri…

2024 Journal of Astrophysics and Astronomy
Gaia 0
Variable circularly polarized radio emission from the young stellar object [BHB2007]-1: Another ingredient of a unique system
DOI: 10.1051/0004-6361/202450568 Bibcode: 2024A&A...690A.303K

Viganò, Daniele; Cleeves, L. Ilsedore; Zurlo, Alice +7 more

The young stellar object [BHB2007]-1 has been extensively studied in the past at radio, millimeter, and infrared wavelengths. It has revealed a gap in the disk and previous observations have claimed possible emission from a sub-stellar object undergoing formation, in correspondence to the disk gap. In this work, we analyzed a set of eight Karl G. …

2024 Astronomy and Astrophysics
Gaia 0