Search Publications

X-ray reprocessing: Through the eclipse spectra of low mass X-ray binaries with XMM-Newton
DOI: 10.1016/j.newast.2023.102109 Bibcode: 2024NewA..10602109A

Paul, Biswajit; Aftab, Nafisa

Eclipsing X-ray binaries make an ideal condition to study reprocessed X-rays, as the X-rays detected during eclipse are purely reprocessed while the much brighter primary X-rays are blocked by the companion star. We carried out a comprehensive study of X-ray reprocessing with four eclipsing Low Mass X-ray Binary (LMXB) systems by comparing X-ray s…

2024 New Astronomy
XMM-Newton 0
Applying machine learning to a nonlinear spectral mixing model for mapping lunar soils composition using CHANDRAYAAN-1 M3 data
DOI: 10.1016/j.pss.2024.105870 Bibcode: 2024P&SS..24405870K

Mall, Urs; Surkov, Yehor; Kaydash, Vadym +4 more

We present a newly developed method which combines the nonlinear spectral mixing model of Shkuratov et al. (1999) with a machine learning algorithm to map the lunar regolith composition using spectral data. The new method performs orders of magnitude faster than the traditionally used numerical optimization approaches, allowing the mapping of rego…

2024 Planetary and Space Science
Chandrayaan-1 0
Cosmological insights into the early accretion of r-process-enhanced stars: II. Dynamical identification of lost members of Reticulum II
DOI: 10.1051/0004-6361/202451837 Bibcode: 2024A&A...692A.130B

Berczik, Peter; Mardini, Mohammad; Ishchenko, Maryna +1 more

Aims. We identify the possible dynamical connection between individual r-process-enhanced stars and the ultra-faint dwarf galaxy Reticulum II based on the current phase-space information for these stars and the dynamical mass-loss model of Reticulum II during its orbital motion for 11.5 Gyr of lookback time. The dynamical orbital modelling togethe…

2024 Astronomy and Astrophysics
Gaia 0
Spectral study of the planetary nebula NGC 2452
DOI: 10.1016/j.newast.2023.102131 Bibcode: 2024NewA..10602131A

Ali, A.; Snaid, S.; Alruhaili, A.

We provide a detailed study for the Galactic planetary nebula (PN) NGC 2452, which has long been suspected to be a member of the Galactic cluster NGC 2453. The present study uses integral field unit (IFU) spectroscopic observations of the PN to explore its physical conditions, chemical abundances, kinematical characteristics, and morphological fea…

2024 New Astronomy
Gaia eHST 0
CMEs evolve in the interplanetary medium to double their predicted geo-effectiveness
DOI: 10.1051/0004-6361/202347552 Bibcode: 2024A&A...686A..23S

Poedts, Stefaan; Mishra, Wageesh; Soni, Shirsh Lata +4 more

Context. We explore the impact of interactions between coronal mass ejections (CMEs) - known as CME-CME interactions - on Earth using remote-sensing and in situ observations and estimate the amplification of the geo-effectiveness of the individual CMEs by a factor of ∼2 due to CME-CME interactions.
Aims: We present 3D reconstructions of inter…

2024 Astronomy and Astrophysics
SOHO 0
Characterization of the Early Dynamics of Solar Coronal Bright Fronts
DOI: 10.48550/arXiv.2404.03396 Bibcode: 2024BlgAJ..41...63N

Stepanyuk, Oleg; Kozarev, Kamen; Nedal, Mohamed +2 more

We present a comprehensive characterization of 26 Coronal Mass Ejection (CME)-driven compressive waves known as Coronal Bright Fronts (CBFs) observed in the low solar corona between 2010 and 2017. These CBFs have been found to be associated with Solar Energetic Particle (SEP) events near Earth, indicating their importance in understanding space we…

2024 Bulgarian Astronomical Journal
SOHO 0
Simultaneous Chandra and HST observations of the quiescent neutron star low-mass X-ray binaries in 47 Tucanae
DOI: 10.1093/mnras/stae1087 Bibcode: 2024MNRAS.531.1653V

van den Berg, M.; Heinke, C. O.; Cohn, H. N. +6 more

We present simultaneous Chandra X-ray Observatory and Hubble Space Telescope observations of three certain (X5, X7, W37) and two likely (X4, W17) quiescent neutron star low-mass X-ray binaries (qLMXBs) in the globular cluster 47 Tuc. We study these systems in the X-ray, optical, and near-ultraviolet (NUV) using the simultaneous data and additional…

2024 Monthly Notices of the Royal Astronomical Society
eHST 0
Correction to: Fundamental parameters for 45 open clusters with Gaia DR2, an improved extinction correction and a metallicity gradient prior
DOI: 10.1093/mnras/stae363 Bibcode: 2024MNRAS.528.6129M

Cantat-Gaudin, T.; Moitinho, A.; Paunzen, E. +4 more

2024 Monthly Notices of the Royal Astronomical Society
Gaia 0
On the Instrumental Discrepancies in Lyman-Alpha Observations of Solar Flares
DOI: 10.1007/s11207-024-02407-7 Bibcode: 2024SoPh..299..162G

Dammasch, Ingolf E.; Milligan, Ryan O.; Greatorex, Harry J.

Despite the energetic significance of Lyman-alpha (Lyα; 1216 Å) emission from solar flares, regular observations of flare related Lyα have been relatively scarce until recently. Advances …

2024 Solar Physics
PROBA-2 0
Mineral detection based on hyperspectral remote sensing imagery on Mars: From detection methods to fine mapping
DOI: 10.1016/j.isprsjprs.2024.09.020 Bibcode: 2024JPRS..218..761K

Zhang, Liangpei; Ke, Tian; Zhong, Yanfei +2 more

Hyperspectral remote sensing is a commonly used technical means for mineral detection on the Martian surface, which has important implications for the study of Martian geological evolution and the study for potential biological signatures. The increasing volume of Martian remote sensing data and complex issues such as the intimate mixture of Marti…

2024 ISPRS Journal of Photogrammetry and Remote Sensing
MEx 0