Velocity field and small scale structure in the L1551 IRS5 jet

Details Velocity field and small scale structure in the L1551 IRS5 jet Velocity field and small scale structure in the L1551 IRS5 jet

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996hst..prop.6411f&link_type=abstract

HST Proposal ID #6411

Astronomy and Astrophysics

Astrophysics

Hst Proposal Id #6411 Binaries And Star Formation

Scientific paper

This is a continuation proposal from cycle 5. Our aim is to image the optical jet emanating from the young stellar object L1551 IRS5 over a period of three cycles. Using two narrow band filters sensitive to high- and low-excitation shocks respectively, we aim to study the time evolution of small scale structures within this object. Ground based observations have already detected the time scale for evolution of this object. HST is going to provide the level of detail necessary for a direct comparison with {existing} hydrodynamical models. Our data will resolve the smallest features observed {optically} so far in an astrophysical jet, and also detect their time evolution. This proposal received already time in cycle 5 with 4 orbits.

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