activity
19942023
most citedA near-infrared study of the NGC 7538 star forming region

79 citations · 2.5k across the 148 of their papers we have counts for

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Showing 2012Show all

10 papers · 1 filter

astro-ph.SR2012★ 38 cited

Optical photometric and polarimetric investigation of NGC 1931

A. K. Pandey, C. Eswaraiah, Saurabh Sharma +7

We present optical photometric and polarimetric observations of stars towards NGC 1931 with the aim to derive the cluster parameters such as distance, reddening, age and luminosity…

astro-ph.SR2012★ 28 cited

Optical and Near-infrared survey of the stellar contents associated with the star-forming Complex Sh2-252

Jessy Jose, A. K. Pandey, K. Ogura +8

We present the analyses of the stellar contents associated with the HII region Sh2-252 using UBVRI photometry, slit and slitless spectroscopy along with the NIR data from 2MASS for…

astro-ph.IM2012★ 9 cited

TIRCAM2: The TIFR Near Infrared Imaging Camera

M. B. Naik, D. K. Ojha, S. K. Ghosh +10

TIRCAM2 (TIFR Near Infrared Imaging Camera - II) is a closed cycle cooled imager that has been developed by the Infrared Astronomy Group at the Tata Institute of Fundamental Resear…

astro-ph.GA2012★ 21 cited

Multi-wavelength study of triggered star formation around mid-infrared bubble N14

L. K. Dewangan, D. K. Ojha

We present multi-wavelength analysis around mid-infrared bubble N14 to probe the signature of triggered star formation as well as the formation of new massive star(s) and/or cluste…

astro-ph.GA2012★ 22 cited

Star formation activity in the Galactic H II region Sh2-297

K. K. Mallick, D. K. Ojha, M. R. Samal +5

We present a multiwavelength study of the Galactic H II region Sh2-297, located in Canis Major OB1 complex. Optical spectroscopic observations are used to constrain the spectral ty…

astro-ph.GA2012★ 30 cited

Triggered star formation around mid-infrared bubbles in G8.14+0.23 H II region

L. K. Dewangan, D. K. Ojha, B. G. Anandarao +2

Mid-infrared (MIR) shells or bubbles around expanding H II regions have received much attention due to their ability to initiate a new generation of star formation. We present mult…