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<HSTProposal
   Phase1ID="569"
   Phase2ID="10649"
   Phase="Phase I"
   AptVersion="Version 14.0 ">
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            Cycle="14"
            IncludeSysInfo="true"
            NotificationAddress="vikram@oddjob.uchicago.edu">
            
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            <SubmissionLog>    Assigned ID: 569
----- Submission 1 (Fri Jan 21 23:56:52 GMT 2005) -----
  Phase I Proposal 569 (grb) successfully submitted.
----- Submission 3 (Sat Jan 22 00:45:47 GMT 2005) -----
  Phase I Proposal 569 (grb) successfully submitted.

----- Submission 4 (Sat Jan 22 00:56:52 GMT 2005) -----
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   <ProposalInformation
      Category="AR"
      PureParallelProposal="false"
      Cycle="14">
      
      <Title>Probing the Circumstellar Environment and Shock Interaction in SN 1987A and Cas A</Title>
      
      <Abstract>Hubble Space Telescope (HST) observations of Supernovae (SNe) and Supernova Remnants have
revolutionized our knowledge of these objects. The spectacular HST images of SN 1987A have
allowed us a real-time look into the impact of the SN shock wave with the surrounding
bipolar nebula, and the development of 'hotspots' along the equatorial ring. HST and other
multi-wavelength data have fostered the development of models for the structure of the
medium surrounding SN 1987A.  HST images of the SN remnant Cas A have revealed an
intricate array of knots and filaments, and confirmed that the ejecta in SNe can be very
clumpy in nature.

These observations can only be understood via detailed, and equally high-resolution,
numerical modeling that takes the evolution of the pre-SN star into account. I propose a
two-year study to investigate the interaction of SN shock waves with the ambient medium
formed by the pre-SN star. This study will differ from others in computing the structure
of the circumstellar medium around the star throughout its evolutionary history. The
mass-loss properties at each timestep in the evolution will be computed from the stellar
properties, which are obtained from the latest stellar evolution models. My
multi-dimensional simulations will provide an important step towards understanding the
complex interaction of the shock-wave with the equatorial ring seen in SN 1987A. I will
study the formation of various instabilities, and their effect on the growth and evolution
of small-scale structures as seen in Cas A. Although my work is motivated primarily by
these two objects, the results will be broadly applicable to a wide variety of phenomena
in which shock wave interaction with the ambient medium is predominant.</Abstract>
      
      <PrincipalInvestigator
         Honorific="Dr."
         FirstName="Vikram"
         LastName="Dwarkadas"
         ESAMember="false"
         UniqueID="6067">
         
         <Address
            Institution="University of Chicago"
            USState="IL"
            Country="USA" />
      </PrincipalInvestigator>
      
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         NextCycle2GyroPrimary="0"
         NextCycle2GyroParallel="0"
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      <Phase1ProposalInformation
         TotalTargets="1"
         Attachment="/home/vikram/grants/stsci/2005/vikram.pdf">
         
         <ScientificCategory>ISM AND CIRCUMSTELLAR MATTER</ScientificCategory>
         
         <ScientificKeyword1
            Keyword="INTERSTELLAR AND INTERGALACTIC MEDIUM" />
         
         <ScientificKeyword2
            Keyword="SUPERNOVA REMNANTS" />
         
         <ScientificKeyword3
            Keyword="SUPERNOVAE" />
         
         <ScientificKeyword4
            Keyword="WINDS/OUTFLOWS/MASS-LOSS" />
         
         <ScientificKeyword5
            Keyword="STELLAR EVOLUTION AND MODELS" />
         
         <ProprietaryPeriod>12</ProprietaryPeriod>
         
         <Budget>139000.00</Budget>
         
         <BudgetExplanation>Budget to be split over 2 years</BudgetExplanation>
         
         <CalibProp>false</CalibProp>
         
         <SpitzerHours>0.0</SpitzerHours>
         
         <SpitzerLarge>false</SpitzerLarge>
         
         <Treasury>false</Treasury>
         
         <Legacy>false</Legacy>
         
         <Theory>true</Theory>
         
         <LargeProgram>false</LargeProgram>
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         <Availability>SUPPORTED</Availability>
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