Frequency andsizedistributiondependenceofvisibleandinfrared extinctionforastronomicalsilicateandgraphitegrains

dc.contributor.authorRoy, Ashim K
dc.contributor.authorSharma, Subodh K
dc.contributor.authorGupta, Ranjan
dc.date.accessioned2012-08-01T12:21:29Z
dc.date.available2012-08-01T12:21:29Z
dc.date.issued2011-10-09
dc.description.abstractIn arecentpaper,thefrequencyandsizedistributiondependenceofextinctionspectra for astronomicalsilicateandgraphitegrainswasanalyzedinthecontextofMRNtype interstellardustmodelsinthefarultravioletandultravioletregions.Thesegrains were takentobehomogeneousspheresfollowingapowerlawsizedistribution.Inthe present workweextendtheanalysisfurthertocoverthevisibleaswellastheinfrared part oftheelectromagneticspectrum.Theanalyticformulaspresentedherealongwith thosegivenintheearlierpaperwouldenableonetoevaluateextinctionforthesegrains withinawiderwavelengthrange1000–22,500 ˚A andanalyzetheobservational interstellarextinctiondatainfargreaterdetailsen_US
dc.identifier.urihttp://hdl.handle.net/11007/1939
dc.language.isoenen_US
dc.publisherJournalofQuantitativeSpectroscopy& RadiativeTransferen_US
dc.subjectInterstellar grainsen_US
dc.subjectExtinction spectrumen_US
dc.subjectSize distributiondependenceen_US
dc.titleFrequency andsizedistributiondependenceofvisibleandinfrared extinctionforastronomicalsilicateandgraphitegrainsen_US
dc.typeArticleen_US

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