Publication data of Nath, Biman B.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion19952000200520102015202020250500100015002000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications199520002005201020152020202502040608010001.534.567.5
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion19952000200520102015202020250510152025
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestConstraining cosmic ray acceleration in young star clusters using multi-wavelength observationsConstraining cosmic ray acceleration in young star clusters using multi-wavel…Dust sputtering by Reverse Shocks in Supernova RemnantsIn a hot bubble: why does superbubble feedback work, but isolated supernovae do not?In a hot bubble: why does superbubble feedback work, but isolated superno…Cosmic ray ionization of the interstellar mediumAGN heating, thermal conduction and Sunyaev-Zeldovich effect in galaxy groups and clustersAGN heating, thermal conduction and Sunyaev-Zeldovich effect in galaxy gr…Did cosmic rays reionize the intergalactic medium?Cosmic backgrounds due to the formation of the first generation of supermassive black holesCosmic backgrounds due to the formation of the first generation of superma…Multiwavelength features of Fermi bubbles as signatures of a Galactic windPrimordial magnetic fields and formation of molecular hydrogenRealistic modelling of wind and supernovae shocks in star clusters: addressing $^{22}$Ne/$^{20}$Ne and other problems in Galactic cosmic raysRealistic modelling of wind and supernovae shocks in star clusters: addressin…On the enrichment of the intergalactic medium by galactic windsEntropy 'floor' and effervescent heating of intracluster gasRadio background and IGM heating due to Pop III supernova explosionsHeating of the intracluster medium by quasar outflowsSelf-regulated black hole accretion, the M - sigma relation, and the growth of bulges in galaxiesSelf-regulated black hole accretion, the M - sigma relation, and the growth of…Photoelectric heating for dust grains at high redshiftsUsing HI to probe large scale structures at z ~ 3Using HI to probe large scale structures at z ~ 3Galactic winds driven by cosmic-ray streaming19952000200520102015202020250500100015002000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Constraining cosmic ray acceleration in young star clusters using multi-wavelength observationsConstraining cosmic ray acceleration in young star clusters using multi-wavel…Dust sputtering by Reverse Shocks in Supernova RemnantsIn a hot bubble: why does superbubble feedback work, but isolated supernovae do not?In a hot bubble: why does superbubble feedback work, but isolated superno…Cosmic ray ionization of the interstellar mediumAGN heating, thermal conduction and Sunyaev-Zeldovich effect in galaxy groups and clustersAGN heating, thermal conduction and Sunyaev-Zeldovich effect in galaxy gr…Did cosmic rays reionize the intergalactic medium?Cosmic backgrounds due to the formation of the first generation of supermassive black holesCosmic backgrounds due to the formation of the first generation of superma…Multiwavelength features of Fermi bubbles as signatures of a Galactic windPrimordial magnetic fields and formation of molecular hydrogenRealistic modelling of wind and supernovae shocks in star clusters: addressing $^{22}$Ne/$^{20}$Ne and other problems in Galactic cosmic raysRealistic modelling of wind and supernovae shocks in star clusters: addressin…On the enrichment of the intergalactic medium by galactic windsEntropy 'floor' and effervescent heating of intracluster gasRadio background and IGM heating due to Pop III supernova explosionsHeating of the intracluster medium by quasar outflowsSelf-regulated black hole accretion, the M - sigma relation, and the growth of bulges in galaxiesSelf-regulated black hole accretion, the M - sigma relation, and the growth of…Photoelectric heating for dust grains at high redshiftsUsing HI to probe large scale structures at z ~ 3Using HI to probe large scale structures at z ~ 3Galactic winds driven by cosmic-ray streaming19952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average1995200020052010201520202025050100150200