activity
20192025
most citedOn the mass accretion rate and infrared excess in Herbig Ae/Be Stars

55 citations · 145 across the 10 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

6 papers · 1 filter

astro-ph.GA2024

Deciphering the properties of UV upturn galaxies in the Virgo cluster

Krishna R. Akhil, Sreeja S Kartha, Namitha Kizhuprakkat +2

The UV upturn refers to the increase in UV flux at wavelengths shorter than 3000 Å observed in quiescent early-type galaxies (ETGs), which still remains a puzzle. In this study, we…

astro-ph.GA2024

Disentangling the association of PAH molecules with star formation : Insights from JWST and UVIT

K. Ujjwal, Sreeja S Kartha, Akhil Krishna R +4

Polycyclic Aromatic Hydrocarbons (PAHs) are ubiquitous complex molecules in the interstellar medium and are used as an indirect indicator of star-formation. On the other hand the u…

astro-ph.GA2023★ 4 cited

DES J024008.08-551047.5:A new member of the polar ring galaxy family

Krishna R. Akhil, Sreeja S Kartha, Blesson Mathew +3

During the visual observations of optical imaging data obtained from the DECaLS, a serendipitous discovery emerged, revealing the presence of a ringed galaxy, DES J024008.08-551047…

astro-ph.GA2023★ 4 cited

What drives the wheels of evolution in NGC 1512? A UVIT study

Thomas Robin, Sreeja S Kartha, Ujjwal Krishnan +4

Environmental and secular processes play a pivotal role in the evolution of galaxies. These can be due to external processes such as interactions or internal processes due to the a…

astro-ph.GA2022★ 11 cited

Understanding the secular evolution of NGC 628 using UVIT

K. Ujjwal, Sreeja S. Kartha, Smitha Subramanian +3

Secular and environmental effects play a significant role in regulating the star formation rate and hence the evolution of the galaxies. Since UV flux is a direct tracer of the sta…

astro-ph.GA2019★ 19 cited

Are Narrow Line Seyfert 1 Galaxies powered by low mass black holes?

Gayathri Viswanath, C S Stalin, Suvendu Rakshit +4

Narrow line Seyfert 1 galaxies (NLS1s) are believed to be powered by accretion of matter onto low mass black holes (BHs) in spiral host galaxies with BH masses M_BH of 10^6 - 10^8…