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Wipro Supernova

Wipro Supernova is the name of a series of high-performance computing (HPC) solutions offered by Wipro Infotech.
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Highly Cited
2015
Highly Cited
2015
A CHANDRASEKHAR MASS PROGENITOR FOR THE TYPE Ia SUPERNOVA REMNANT 3C 397 FROM THE ENHANCED ABUNDANCES OF NICKEL AND MANGANESE
Despite decades of intense efforts, many fundamental aspects of Type Ia supernovae (SNe Ia) remain elusive. One of the major open… 
Highly Cited
2010
Highly Cited
2010
EXPANSION VELOCITY OF EJECTA IN TYCHO's SUPERNOVA REMNANT MEASURED BY DOPPLER BROADENED X-RAY LINE EMISSION
We show that the expansion of ejecta in Tycho's supernova remnant (SNR) is consistent with a spherically symmetric shell, based… 
2010
2010
Time-dependent particle acceleration in supernova remnants in different environments
We simulate time-dependent particle acceleration in the blast wave of a young supernova remnant (SNR), using a Monte Carlo… 
Highly Cited
2009
Highly Cited
2009
MAGNETIC AMPLIFICATION BY MAGNETIZED COSMIC RAYS IN SUPERNOVA REMNANT SHOCKS
X-ray observations of synchrotron rims in supernova remnant (SNR) shocks show evidence of efficient electron acceleration and… 
2007
2007
The Formation of a Cooling Layer in a Partially Optically Thick Shock
The mechanics of a radiative shock which has “collapsed,” or been compressed to high density, via radiative cooling is discussed… 
Highly Cited
2003
Highly Cited
2003
Submitted to ApJ Letters
  • 2003
  • Corpus ID: 6059959
Highly Cited
1998
Highly Cited
1998
OH (1720 MHz) Masers as Signposts of Molecular Shocks
We present observations of molecular gas made with the 15 m James Clark Maxwell Telescope toward the sites of OH (1720 MHz… 
Highly Cited
1998
Highly Cited
1998
Radio Emission from a Young Supernova Remnant Interacting with an Interstellar Cloud: Magnetohydrodynamic Simulation with Relativistic Electrons
We present two-dimensional MHD simulations of the evolution of a young Type Ia supernova remnant (SNR) during its interaction… 
Highly Cited
1992
Highly Cited
1992
Identification of features due to H3 + in the infrared spectrum of supernova 1987A
THE molecular ion H3 + occupies a central position in theoretical models of interstellar chemistry1,2. It forms readily in… 
1987
1987
Light-curve models for supernova SN1987A in the Large Magellanic Cloud
Neutrino bursts from the supernova SN1987A have been reported1–3 which provide qualitatively new information as to the time… 
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