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Deeply comprehensive astrometric, photometric, and kinematic studies of the three OCSN open clusters with Gaia DR3
DOI: 10.1007/s12036-025-10044-0 Bibcode: 2025JApA...26...21E

Elsanhoury, W. H.; Çınar, D. C.; Haroon, A. A. +1 more

In this study, we considered the optical wavelength of Gaia Data Release 3 (DR3) to analyze poorly studied three newly open star clusters, namely OCSN 203, OCSN 213, and OCSN 244 clusters with ASTECA code. Here, we identified 227, 200, and 551 candidates with highly probable (P

2025 Journal of Astrophysics and Astronomy
Gaia 3
X-ray study of WR 48-6: A possible colliding wind binary: X-ray study of WR 48-6: a possible colliding...
DOI: 10.1007/s12036-025-10039-x Bibcode: 2025JApA...46...16J

Tej, Anandmayee; Pandey, Jeewan C.; Jadoliya, Vishal

This paper presents an investigation of the X-ray emission associated with the Wolf–Rayet star, WR 48-6, using observations from the XMM-Newton and Chandra X-ray telescopes covering two epochs separated by eleven months. The X-ray spectrum of WR 48-6 is well explained by a two-temperature plasma model, with cool and hot plasma temperatures of

2025 Journal of Astrophysics and Astronomy
XMM-Newton 0