Publications (8)
Reaction-Drift Model for Switching Transients in PrCaMnO Based Resistive RAM
A. Khanna, S. Prasad, N. Panwar +1
Earlier, the DC hole-current modeling of PCMO RRAM by drift-diffusion (DD) including self-heating (SH) in TCAD (but without ionic transport) was able to explain the experimentally…
Space Charge Limited Current with Self-heating in PrCaMnO based RRAM
I. Chakraborty, N. Panwar, A. Khanna +1
Space Charge Limited Current (SCLC) based conduction has been identified for PCMO-based RRAM devices based on the observation that where . A critical…
MAGIC gamma-ray and multifrequency observations of flat spectrum radio quasar PKS 1510-089 in early 2012
MAGIC Collaboration, J. AleksiÄ, S. Ansoldi +218
Among more than fifty blazars detected in very high energy (VHE, E>100GeV) gamma-rays, only three belong to the subclass of Flat Spectrum Radio Quasars (FSRQs). MAGIC observed FSRQ…
Variability of the blazar 4C 38.41 (B3 1633+382) from GHz frequencies to GeV energies
C. M. Raiteri, M. Villata, P. S. Smith +74
The quasar-type blazar 4C 38.41 (B3 1633+382) experienced a large outburst in 2011, which was detected throughout the entire electromagnetic spectrum. We present the results of low…
Variability of young stellar objects in the star-forming region Pelican Nebula
A. Bhardwaj, N. Panwar, G. J. Herczeg +2
We observed a field of in the star-forming region Pelican Nebula (IC 5070) at wavelengths for 90 nights spread over one year in 2012-2013. More than 250 epoc…
The disintegrating old open cluster Czernik 3
Saurabh Sharma, Arpan Ghosh, D. K. Ojha +6
We have performed a detailed analysis of the Czernik 3 (Cz3) open cluster by using deep near-infrared photometry taken with TIRCAM2 on 3.6m Devasthal optical telescope along with t…
Characterization of the Praesepe Star Cluster by Photometry and Proper Motions with 2MASS, PPMXL, and Pan-STARRS
P. F. Wang, W. P. Chen, C. C. Lin +31
Membership identification is the first step to determine the properties of a star cluster. Low-mass members in particular could be used to trace the dynamical history, such as mass…
A Comprehensive Study of the Young Cluster IRAS 05100+3723: Properties, Surrounding Interstellar Matter, and Associated Star Formation
R. K. Yadav, M. R. Samal, E. Semenko +13
We present a comprehensive multiwavelength investigation of a likely massive young cluster `IRAS 05100+3723' and its environment with the aim to understand its formation history an…