most citedThe MLP Distribution: A Modified Lognormal Power-Law Model for the Stellar Initial Mass Function

36 citations · 53 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2017

From Molecular Clouds to the IMF: Spatial and Temporal Effects

Shantanu Basu, Sayantan Auddy

We review star formation in molecular clouds and describe why magnetic fields may be important and how they can influence filamentary structure and the column density probability d…

astro-ph.GA201716 cited

The Effect of Magnetic Fields and Ambipolar Diffusion on the Column Density Probability Distribution Function in Molecular Clouds

Sayantan Auddy, Shantanu Basu, Takahiro Kudoh

Simulations generally show that non-self-gravitating clouds have a lognormal column density () probability distribution function (PDF), while self-gravitating clouds with active…

astro-ph.GA20171 cited

Magnetic Ribbons: A Minimum Hypothesis Model for Filaments

Sayantan Auddy, Shantanu Basu, Takahiro Kudoh

We develop a magnetic ribbon model for molecular cloud filaments. These result from turbulent compression in a molecular cloud in which the background magnetic field sets a preferr…

quant-ph2017

The Anomalous Magnetic Moment of a Photon Propagating in a Magnetic Field

Julian W. Mielniczuk, Darrell Lamm, Sayantan Auddy +1

We analyze the spectrum of the Hamiltonian of a photon propagating in a strong magnetic field , where Gauss…

astro-ph.CO2015

Gravitational Wave Background in the Quasi-Steady State Cosmology

J. V. Narlikar, S. V. Dhurandhar, R. G. Vishwakarma +2

This paper calculates the expected gravitational wave background (GWB) in the quasi-steady state cosmology (QSSC). The principal sources of gravitational waves in the QSSC are the…

astro-ph.SR201536 cited

The MLP Distribution: A Modified Lognormal Power-Law Model for the Stellar Initial Mass Function

Shantanu Basu, M. Gil, Sayantan Auddy

This work explores the mathematical properties of a distribution introduced by Basu & Jones (2004), and applies it to model the stellar initial mass function (IMF). The distributio…