Search Publications

A Search for X-Ray/UV Correlation in the Reflection-dominated Seyfert 1 Galaxy Markarian 1044
DOI: 10.3847/1538-4357/acf464 Bibcode: 2023ApJ...958...46B

Jithesh, V.; Medhi, Biman J.; Misra, Ranjeev +3 more

Correlated variability between coronal X-rays and disk optical/UV photons provides a very useful diagnostic of the interplay between the different regions around an active galactic nucleus (AGN) and how they interact. AGNs that reveal strong X-ray reflection in their spectra should normally exhibit optical/UV to X-ray correlation consistent with r…

2023 The Astrophysical Journal
XMM-Newton 2
Orbit determination for the binary Cepheid V1344 Aql
DOI: 10.1051/0004-6361/202347360 Bibcode: 2023A&A...680A..89C

Szabados, L.; Cseh, B.; Kovács, J. +4 more

Context. Binary Cepheids play an important role in the investigation of the calibration of the classical Cepheid period-luminosity relationship. Therefore, a thorough study of individual Cepheids belonging to binary systems is necessary.
Aims: Our aim is to determine the orbit of the binary system V1344 Aql using newly observed and earlier pu…

2023 Astronomy and Astrophysics
INTEGRAL 2
Star Structure of the Northern Part of the Orion Sword Region
DOI: 10.1134/S1063772923040042 Bibcode: 2023ARep...67..336V

Vereshchagin, S. V.; Chupina, N. V.

According to the data of the Gaia DR3 catalogs, the belonging of the stars of group 189 ([1]), located in the northern part of the Orion Sword region, to the open star cluster (OSC) NGC 1977 was analyzed. To do this, the revision of the stellar composition of the northern part of the Orion Sword region (around the center of the OSC NGC 1977) was c…

2023 Astronomy Reports
Gaia 2
Atmospheric Pressure and Molecular Cloud Formation in Early-type Galaxies
DOI: 10.3847/1538-4357/acb53f Bibcode: 2023ApJ...944...69B

McNamara, B. R.; Russell, H. R.; Edge, A. C. +3 more

A strong correlation between atmospheric pressure and molecular gas mass is found in central cluster galaxies and early-type galaxies. This trend and a similar trend with atmospheric gas density would naturally arise if the molecular clouds condensed from hot atmospheres. Limits on the ratio of molecular to atomic hydrogen in these systems exceed …

2023 The Astrophysical Journal
XMM-Newton 2
Deep and shallow crustal structure control on the late-stage volcanism in Syria Planum (Mars)
DOI: 10.1016/j.jvolgeores.2023.107830 Bibcode: 2023JVGR..43907830P

Pozzobon, Riccardo; Mazzarini, Francesco; Isola, Ilaria

Long-lasting widespread volcanism in Mars is testified by the Tharsis volcanic province, one of the largest volcanic provinces with the largest shield volcanoes of the Solar System. However, volcanism on Mars is characterized also by the occurrence of broad volcanic fields, either in the form of small lava shields or monogenic volcanic cones. The …

2023 Journal of Volcanology and Geothermal Research
MEx 2
WISE Green Objects (WGOs): The Massive Star Candidates in the Whole Galactic Plane (∣b∣ < 2°)
DOI: 10.3847/1538-4365/aca325 Bibcode: 2023ApJS..264...24Z

Yuan, Jing-Hua; Zhang, Guo-Yin; Zhang, Chang +1 more

Massive young stellar objects (MYSOs) play a crucial role in star formation. Given that MYSOs were previously identified based on the extended structure and the observational data for them is limited, screening the Wide-field Infrared Survey Explorer (WISE) objects showing green features (for the common coding of the 4.6 µm band as the green…

2023 The Astrophysical Journal Supplement Series
Herschel 2
Transverse Vertical Oscillations During the Contraction and Expansion of Coronal Loops
DOI: 10.3847/1538-4357/acd5cf Bibcode: 2023ApJ...951..126Z

Li, Qiao; Zhang, Qingmin; Li, Chuan +5 more

In this paper, we carry out a detailed analysis of the M1.6 class eruptive flare occurring in NOAA active region 13078 on 2022 August 19. The flare is associated with a fast coronal mass ejection (CME) propagating in the southwest direction with an apparent speed of ~926 km s-1. Meanwhile, a shock wave is driven by the CME at the flank.…

2023 The Astrophysical Journal
SOHO 2
Detailed analysis of the variable star population in the globular cluster NGC 7006
DOI: 10.1093/mnras/stac3650 Bibcode: 2023MNRAS.519.2451A

Arellano Ferro, A.; Muneer, S.; Bustos Fierro, I. H. +3 more

A 5-yr CCD photometric VI time series of NGC 7006 is employed to perform a detailed analysis of the known population of variable stars. In the process, we have corrected inconsistent classifications, sky coordinates and found 10 new cluster member variables. An independent reddening estimate with a value E(B-V) = 0.08 ± 0.05 is made. Using Fourier…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 2
Accelerating Multiframe Blind Deconvolution via Deep Learning
DOI: 10.1007/s11207-023-02185-8 Bibcode: 2023SoPh..298...91A

Asensio Ramos, Andrés; Kuckein, Christoph; Esteban Pozuelo, Sara

Ground-based solar-image restoration is a computationally expensive procedure that involves nonlinear optimization techniques. The presence of atmospheric turbulence produces perturbations in individual images that make it necessary to apply blind deconvolution techniques. These techniques rely on the observation of many short-exposure frames that…

2023 Solar Physics
Herschel 2
The nature of 500 micron risers - II. Multiplicities and environments of sub-mm faint dusty star-forming galaxies
DOI: 10.1093/mnras/stac3486 Bibcode: 2023MNRAS.519..709C

Pérez-Fournon, I.; Clements, D. L.; Riechers, D. +6 more

We present Submillimeter Common User Bolometer Array 2 (SCUBA-2) and Submillimeter Array (SMA) follow-up observations of four candidate high-redshift dusty star-forming galaxies, selected as sources with rising spectral energy distributions in the 250, 350, and 500 µm Herschel SPIRE bands. Previous SMA observations showed no counterparts to …

2023 Monthly Notices of the Royal Astronomical Society
Herschel 2