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20242026
most citedNon-Linear Solar EUV-Driven Sodium Release from the Lunar Surface: A Contrast to the Linear PSD Model

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astro-ph.SR2026

A Novel Approach to Identify Unseen Companions: An In-Depth study of GDR3 220_28

T. B. Cysil, Blesson Mathew, B. Shridharan +6

Emission lines in the spectrum and the excess seen in the spectral energy distribution (SED) at infrared (IR) wavelengths serve as crucial indicators of accretion activity and the…

astro-ph.SR2026

A comprehensive multi-wavelength study of two X-ray emitting Be stars

Hema Anilkumar, Blesson Mathew, Savithri H. Ezhikode +4

We present a multi-wavelength study of two X-ray-emitting Be stars, CXOU J052218.4+332820 (Star 1) and CXOU J052304.2+332846 (Star 2), identified from the LAMOST DR5 Hot emission-l…

astro-ph.SR2026

ROCKETS I: Investigating the Impact of the Rocket Effect on Two Nearby Young Open Clusters Encased in Infrared Bubbles

R. Arun, G. Maheswar, Annapurni Subramaniam +5

We introduce ROCKETS (Rocket-driven Cluster Kinematics & Triggered Star-formation), a Gaia based programme investigating kinematic fingerprints of stellar feedback or rocket effect…

astro-ph.SR2026

Investigating the properties of nearby young moving groups using GaiaDR3

Mamta Lad, Ujjwal Krishnan, Blesson Mathew +4

Moving groups, which are gravitationally unbound collections of stars spread over large portions of the sky, pose challenges to their identification. Analyzing the three-dimensiona…

astro-ph.SR2026

A multi-epoch spectral and photometric study to understand the nature of the interesting Be star candidate HD 249179

Suman Bhattacharyya, Blesson Mathew, S Muneer +2

HD 249179, a B5 star with unclear classification as either a classical Be star or a high-mass X-ray binary (HMXB) system, is investigated using the first multi-epoch spectral and p…