activity
20022019
most citedStudy of the plutino object (208996) 2003 AZ84 from stellar occultations: size, shape and topographic features

50 citations · 156 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.SR2019★ 7 cited

Characteristics of the Solar Coronal Line Profiles from Fabry-Perot Interferometric Observations

Maya Prabhakar, K. P. Raju, T. Chandrasekhar

This article reports the analysis of a set of Fabry-Perot interferograms that were studied to probe the physical parameters of the inner solar corona. The observations were carried…

astro-ph.EP2017★ 50 cited

Study of the plutino object (208996) 2003 AZ84 from stellar occultations: size, shape and topographic features

A. Dias-Oliveira, B. Sicardy, J. L. Ortiz +60

We present results derived from four stellar occultations by the plutino object (208996) 2003~AZ, detected at January 8, 2011 (single-chord event), February 3, 2012 (multi-c…

astro-ph.GA2015★ 25 cited

Star formation towards the southern Cometary HII region IRAS 17256-3631

V. S. Veena, S. Vig, A. Tej +4

IRAS 17256-3631 is a southern Galactic massive star forming region located at a distance of 2 kpc. In this paper, we present a multiwavelength investigation of the embedded cluster…

astro-ph.SR2014★ 1 cited

Possible spatial asymmetry in semi-regular variable UZ Arietis

Tapas Baug, T. Chandrasekhar, Shashikiran Ganesh

Semi-regular variables (SRVs) though closely related to Mira variables, are a less studied class of AGB stars. While asymmetry in the brightness distribution of many Mira variables…

astro-ph.SR2013★ 1 cited

Analysis of the solar coronal green line profiles from eclipse observations

Maya Prabhakar, K. P. Raju, T. Chandrasekhar

Analysis of the solar coronal green line profiles reveals information regarding the physical conditions of the solar corona like temperature, density, Doppler velocity, non-thermal…

astro-ph.SR2013★ 4 cited

Noise reduction methods in analysis of near infrared lunar occultation light curves for high angular resolution measurements

Tapas Baug, Thyagarajan Chandrasekhar

Lunar occultation (LO) technique in the near-infrared provides angular resolution down to milliarcseconds on the occulted source even with ground-based 1m class telescopes. LO obse…