activity
20122024
most citedMolecular scale height in spiral galaxies

30 citations · 93 across the 9 of their papers we have counts for

collaborators

15 papers

astro-ph.GA20218 cited

A Comparison of the UV and HI Properties of the Extended UV (XUV) Disk Galaxies NGC 2541, NGC 5832 and ESO406-042

M. Das, Yadav, J. +11

We present a UV study of 3 extended UV (XUV) galaxies that we have observed with the UVIT and the GMRT. XUV galaxies show filamentary or diffuse star formation well beyond their op…

astro-ph.GA2021

Comparing the Inner and Outer Star Forming Complexes in the Nearby Spiral Galaxies NGC 628, NGC 5457 and NGC 6946 using UVIT Observations

Jyoti Yadav, Mousumi Das, Narendra Nath Patra +5

We present a far-UV (FUV) study of the star-forming complexes (SFCs) in three nearby galaxies using the Ultraviolet Imaging Telescope (UVIT). The galaxies are close to face-on and…

astro-ph.GA2020

Thick disc molecular gas fraction in NGC 6946

Narendra Nath Patra

Several recent studies reinforce the existence of a thick molecular disc in galaxies along with the dynamically cold thin disc. Assuming a two-component molecular disc, we model th…

astro-ph.GA2020

HI scale height in spiral galaxies

Narendra Nath Patra

We model the galactic discs of seven nearby large spiral galaxies as three-component systems consist of stars, molecular gas, and atomic gas in vertical hydrostatic equilibrium. We…

astro-ph.CO202025 cited

The All-Sky SignAl Short-Spacing INterferometer (ASSASSIN) I: Global sky measurements with the Engineering Development Array-2

B. McKinley, C. M. Trott, M. Sokolowski +5

Aiming to fill a crucial gap in our observational knowledge of the early Universe, experiments around the world continue to attempt to verify the claimed detection of the redshifte…

astro-ph.GA20204 cited

New HI observations of KK 69. Is KK 69 a dwarf galaxy in transition?

J. Saponara, B. S. Koribalski, N. N. Patra +1

We present new HI data of the dwarf galaxy KK 69, obtained with the Giant Metrewave Radio Telescope (GMRT) with a signal-to-noise ratio that almost double previous observations. We…