activity
20182022
most citedOn the mass accretion rate and infrared excess in Herbig Ae/Be Stars

55 citations · 127 across the 5 of their papers we have counts for

collaborators

9 papers

astro-ph.SR20222 cited

Study of Classical Be stars in open clusters older than 100 Myr

Madhu Kashyap Jagadeesh, Blesson Mathew, K. T. Paul +3

We performed the slitless spectroscopic survey to identify Classical (CBe) stars in open clusters older than 100 Myr. Observing a sample of 71 open clusters, we identified 13 CBe s…

astro-ph.SR202019 cited

Identification of new Classical Ae stars in the Galaxy using LAMOST DR5

R. Anusha, Blesson Mathew, B. Shridharan +6

We report the first systematic study to identify and characterize a sample of classical Ae stars in the Galaxy. The spectra of these stars were retrieved from the A-star catalog us…

astro-ph.SR202014 cited

Optical spectroscopy of Galactic field Classical Be stars

Gourav Banerjee, Blesson Mathew, K. T. Paul +3

In this study, we analyze the emission lines of different species present in 118 Galactic field classical Be stars in the wavelength range of 3800 - 9000 Å. We re-estimated the ext…

astro-ph.GA2020

More insights into bar quenching. Multi-wavelength analysis of four barred galaxies

Koshy George, P. Joseph, C. Mondal +3

The underlying nature of the process of star formation quenching in the central regions of barred disc galaxies that is due to the action of stellar bar is not fully understood. We…

astro-ph.GA2019

Significance of bar quenching in the global quenching of star formation

Koshy George, Smitha Subramanian, K. T. Paul

The suppression of star formation in the inner kiloparsec regions of barred disk galaxies due to the action of bars is known as bar quenching. We investigate here the significance…

astro-ph.SR201955 cited

On the mass accretion rate and infrared excess in Herbig Ae/Be Stars

R. Arun, Blesson Mathew, P. Manoj +5

The present study makes use of the unprecedented capability of the Gaia mission to obtain the stellar parameters such as distance, age, and mass of HAeBe stars. The accuracy of Gai…