output
20022024
most citedFlavour physics of leptons and dipole moments

378 citations

Showing 2024Show all

12 papers · 1 filter

astro-ph.SR20241 cited

The Gaia Ultracool Dwarf Sample -- IV. GTC/OSIRIS optical spectra of Gaia late-M and L dwarfs

W. J. Cooper, H. R. A. Jones, R. L. Smart +20

As part of our comprehensive, ongoing characterisation of the low-mass end of the main sequence in the Solar neighbourhood, we used the OSIRIS instrument at the 10.4 m Gran Telesco…

astro-ph.GA2024

Peering into the Heart of the Giant Molecular Cloud G148.24+00.41: A Deep Near-infrared View of the Newly Hatched Cluster FSR 655

Vineet Rawat, M. R. Samal, D. K. Ojha +5

We present a detailed near-infrared study of an embedded cluster located in the hub of the giant molecular cloud G148.24+00.41 of mass 10 , with the TANSPEC inst…

astro-ph.GA20244 cited

Linear polarization study of open clusters towards the anticenter direction: Signature of the spiral arms

Namita Uppal, Shashikiran Ganesh, Vincent Pelgrims +2

Our objective is to investigate the distribution of dust and associated large-scale structures of the Galaxy using optical linear polarization measurements of various open clusters…

astro-ph.SR20248 cited

On the Response of the Transition Region and the Corona to Rapid Excursions in the Chromosphere

Ravi Chaurasiya, Ankala Raja Bayanna, R. E. Louis +2

Spicules are the thin hair/grass-like structures that are prominently observed at the chromospheric solar limb. It is believed that fibrils and rapid blueshifted and redshifted exc…

astro-ph.HE2024

Study of Wolf-Rayet stars using uGMRT

Anindya Saha, Anandmayee Tej, Santiago del Palacio +4

In recent years, systems involving massive stars with large wind kinetic power have been considered as promising sites for investigating relativistic particle acceleration in low r…

astro-ph.SR2024

A dusty rain falls on the nova V959 Monocerotis

A. Evans, D. P. K. Banerjee, W. P. Varricatt +1

We present archival and ground-based infrared observations of the gamma-ray-emitting nova V959 Mon, covering the period 100-4205 days after the 2012 eruption. We use these data to…