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X-ray emission of the radio-loud quasar SDSS J121426.52+140258.9: independent variations between optical/UV and X-ray emission
DOI: 10.1093/mnras/stac3475 Bibcode: 2023MNRAS.519..909Z

Anjum, Muhammad S.; Liao, Mai; Gu, Minfeng +1 more

To understand the X-ray emission of active galactic nuclei (AGNs), we explored the optical-to-X-ray variation correlation of a radio-loud quasar (RLQ) SDSS J121426.52+140258.9 (hereafter J1214+1402) with multi-epoch observations by the Swift and XMM-Newton telescopes. With the historical multiband data, we found that the infrared-to-X-ray flux of …

2023 Monthly Notices of the Royal Astronomical Society
XMM-Newton 0
Differences between the globular cluster systems of the Virgo and Fornax galaxy clusters
DOI: 10.1093/mnras/stac3161 Bibcode: 2023MNRAS.519..613D

Mieske, Steffen; Dabringhausen, Jörg; Fellhauer, Michael

It is well-known that Globular cluster systems are different among galaxies. Here, we test to which degree these differences remain on the scale of galaxy clusters by comparing the globular clusters (GCs) in optical surveys of the Virgo galaxy cluster (ACSVCS) and the ACS Fornax galaxy cluster (ACSFCS) in Kolmogorov-Smirnoff Tests. Both surveys we…

2023 Monthly Notices of the Royal Astronomical Society
eHST 0
Apsidal motion and absolute parameters of GV Nor and V881 Sco based on mid-resolution spectroscopy and TESS photometry
DOI: 10.1093/mnras/stac3738 Bibcode: 2023MNRAS.519.4699S

Erdem, Ahmet; Sürgit, Derya; Engelbrecht, Chris A. +5 more

The veracity of stellar evolution models and theoretical internal structure constants may be subjected to stringent tests by using physical parameters obtained from spectroscopic and photometric observations of eclipsing binary systems that exhibit apsidal motion. Two eclipsing binary stars from the southern hemisphere with no prior published spec…

2023 Monthly Notices of the Royal Astronomical Society
Gaia INTEGRAL 0
Supermassive black holes in a mass-limited galaxy sample
DOI: 10.1093/mnras/stad2771 Bibcode: 2023MNRAS.526.1095B

Drinkwater, Michael J.; Côté, Patrick; Ferrarese, Laura +8 more

The observed scaling relations between supermassive black hole masses and their host galaxy properties indicate that supermassive black holes influence the evolution of galaxies. However, the scaling relations may be affected by selection biases. We propose to measure black hole masses in a mass-limited galaxy sample including all non-detections t…

2023 Monthly Notices of the Royal Astronomical Society
eHST 0
A statistical study of trans-equatorial loops from 2006 to 2020
DOI: 10.1093/mnras/stad2224 Bibcode: 2023MNRAS.524.5880Y

Pevtsov, Alexei A.; Xue, Zhike; Su, Jiangtao +5 more

We studied trans-equatorial loops (TLs) statistically from December 2006 to 2020. During this period, 160 TLs were identified, and 12 per cent of all active regions are connected by TLs. The result shows that 74 per cent of TLs are connected to regions of preceding magnetic polarity (PTLs), and only 26 per cent of TLs are connected to regions of f…

2023 Monthly Notices of the Royal Astronomical Society
Hinode SOHO 0
A photodissociation region (PDR) model grid in planetary nebula paradigm: dependency of C and O fine structure line emission and PDR thermal structure on central star radiation and nebular dust composition
DOI: 10.1093/mnras/stad1129 Bibcode: 2023MNRAS.523..498B

Das, Ramkrishna; Bandyopadhyay, Rahul

We compute a grid of photodissociation region (PDR) models. The varying parameters of the grid include effective temperature (Teff) and luminosity (L) of the radiation source, density (nH) of the nebula, PDR depth from the nebular ionization front (ΔrPDR), and densities of polycyclic aromatic hydrocarbon (PAH) mole…

2023 Monthly Notices of the Royal Astronomical Society
Herschel ISO 0
Variation of temperature and non-thermal velocity with height in fan loops
DOI: 10.1093/mnras/stad2359 Bibcode: 2023MNRAS.525.1657S

Tripathi, Durgesh; Sharma, Aishawnnya

We study the variation of temperature and non-thermal velocity with height in fan loops. For this purpose, we have used the observations recorded by the Extreme Ultraviolet Imaging Spectrometer onboard Hinode. We have employed the emission measure (EM)-loci method to estimate the temperatures of different coronal fan loops and then compute the non…

2023 Monthly Notices of the Royal Astronomical Society
Hinode 0