Search Publications

Exploring the relationship between X-ray binaries and compact star clusters (I): NGC 4490 and NGC 4214
DOI: 10.1093/mnras/stae618 Bibcode: 2024MNRAS.529.1507A

Akyuz, A.; Aksaker, N.; Allak, S. +3 more

We conducted a study to investigate the relationship between X-ray binaries (XRBs) and compact star clusters in the nearby star-forming galaxies NGC 4490 and NGC 4214. By analysing archival data from Chandra, we identified a total of 32 XRBs with X-ray luminosities Lx > 1036 erg s-1 in both galaxies. Utilizing d…

2024 Monthly Notices of the Royal Astronomical Society
eHST 1
X-ray flux and spectral variability of the blazar OJ 287 with Suzaku
DOI: 10.1093/mnras/stae1722 Bibcode: 2024MNRAS.532.3285Z

Gupta, Alok C.; Wiita, Paul J.; Xu, Haiguang +4 more

We present analyses of Suzaku XIS light curves and spectra of the BL Lac object OJ 287 with observations positioned primarily around proposed recurrent optical outbursts. The first two observations were performed in 2007 April 10-13 (epoch 1) and 2007 November 7-9 (epoch 2) that, respectively, correspond to a low and a high optical state and which…

2024 Monthly Notices of the Royal Astronomical Society
Suzaku 1
HD 28185 revisited: an outer planet, instead of a brown dwarf, on a Saturn-like orbit
DOI: 10.1093/mnras/stae2336 Bibcode: 2024MNRAS.535...90V

Vanderburg, Andrew; Wittenmyer, Robert A.; Huang, Chelsea X. +3 more

As exoplanet surveys reach ever-higher sensitivities and durations, planets analogous to the Solar system giant planets are increasingly within reach. HD 28185 is a Sun-like star known to host a $m\sin i=6~M_\mathrm{ J}$ planet on an Earth-like orbit; more recently,…

2024 Monthly Notices of the Royal Astronomical Society
Gaia Hipparcos 1
Evidence of dark contents in the centre of NGC 6517
DOI: 10.1093/mnras/stad3598 Bibcode: 2024MNRAS.527.7743X

Xie, Yi; Zhang, Liyun; Lian, Yujie +3 more

Millisecond pulsars can serve as effective probes to investigate the presence of intermediate-mass black holes (IMBHs) within Galactic globular clusters (GCs). Based on the standard structure models for GCs, we conduct simulations to analyse the distributions of pulsar accelerations within the central region of NGC 6517. By comparing the measured …

2024 Monthly Notices of the Royal Astronomical Society
eHST 1
Deciphering the evolution of thermodynamic properties and their connection to the global kinematics of high-speed coronal mass ejections using FRIS model
DOI: 10.1093/mnras/stae2523 Bibcode: 2024MNRAS.535.2585K

Wang, Yuming; Nieves-Chinchilla, Teresa; Mishra, Wageesh +3 more

Most earlier studies have been limited to estimating the kinematic evolution of coronal mass ejections (CMEs), and only limited efforts have been made to investigate their thermodynamic evolution. We focus on the interplay of the thermal properties of CMEs with their observed global kinematics. We implement the Flux rope Internal State model to es…

2024 Monthly Notices of the Royal Astronomical Society
SOHO 1
Charging effects on Rosetta dust measurements
DOI: 10.1093/mnras/stae2231 Bibcode: 2024MNRAS.534.2119H

Deca, Jan; Horányi, Mihály

Dust particles released from comet 67P/Churyumov-Gerasimenko collect electrostatic charges. Their motion is influenced by the electric fields induced by the flow of the solar wind and by the charging of the Rosetta spacecraft itself. Dust grains with sufficiently low tensile strength might even be destroyed en route from the nucleus to Rosetta. A …

2024 Monthly Notices of the Royal Astronomical Society
Rosetta 1
Time evolution of X-ray bright points observed with NuSTAR
DOI: 10.1093/mnras/stae417 Bibcode: 2024MNRAS.528.6398P

Krucker, Säm; White, Stephen M.; Grefenstette, Brian W. +5 more

We present analysis on two X-ray bright points observed over several hours during the recent solar minimum (2020 February 21 and 2020 September 12-13) with the Nuclear Spectroscopic Telescope Array (NuSTAR), a sensitive hard X-ray imaging spectrometer. This is so far the most detailed study of bright points in hard X-rays, emission which can be us…

2024 Monthly Notices of the Royal Astronomical Society
Hinode 1
A statistical approach to polarimetric and photometric investigation of the intermediate-age open cluster NGC 1912
DOI: 10.1093/mnras/stae1476 Bibcode: 2024MNRAS.532.1241B

Biswas, Samrat; Medhi, Biman J.; Deb, Sushmita +3 more

This paper presents a comprehensive multiwavelength investigation of the intermediate-age open cluster NGC 1912. We identified 401 member stars for NGC 1912 using K-nearest neighbour and Gaussian Mixture Model machine learning techniques. The fundamental parameters determined for the cluster are metallicity (z) = 0.0141 $\pm$ 0.0006, log(age) = 8.…

2024 Monthly Notices of the Royal Astronomical Society
AKARI Gaia Herschel 1
On stellar migration from Andromeda to the Milky Way
DOI: 10.1093/mnras/stae712 Bibcode: 2024MNRAS.529.3816G

Schwarz, Dominik J.; Fairbairn, Malcolm; Gülzow, Lukas

Recent Gaia observations suggest that some hypervelocity stars (HVSs) might originate from outside the Galaxy. We ask whether these HVSs could come from as far as Andromeda. Therefore, we simulate HVSs originating in Andromeda with initial conditions based on attributes of high-velocity stars measured in the Milky Way and a simple model for the gr…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 1
Long-term orbital evolution of dimorphos boulders and implications on the origin of meteorites
DOI: 10.1093/mnras/stae464 Bibcode: 2024MNRAS.528.6660F

Carbognani, A.; Fenucci, M.

By using recent observations of the Dydimos-Dimorphos system from the Hubble Space Telescope, 37 boulders with a size of 4 to 7 m ejected from the system during the impact with the DART spacecraft were identified. In this work, we studied the orbital evolution of a swarm of boulders with a similar size to that of the detected ones. By using recent…

2024 Monthly Notices of the Royal Astronomical Society
eHST 1