!  File:  1074C.PROP
!  Database:  PEPDB
!  Date:  16-FEB-1994:00:43:42

coverpage:

  title_1:         OORT CLOUD IN PLANETARY NEBULAE-CYCLE9
    sci_cat:       INTERSTELLAR MEDIUM
    proposal_for:  GTO/OS
    pi_title:      PROF.
    pi_fname:      C.
    pi_mi:         R.
    pi_lname:      O'DELL
    pi_inst:       RICE UNIVERSITY
    pi_country:    USA
    pi_phone:      713-527-8101 X 3633
    keywords_1:    PLANETARY NEBULAE
    hours_pri:     2.70
    num_pri:       2
    wf_pc:         X
    pi_position:   PROF. SP.PHYS.ASTR.
! end of coverpage

abstract:

    line_1:        Under the assumption that the Oort Cloud of Comets is a common feature of stars
    line_2:        with planetary systems and the planetary nebulae nuclei are advanced stages of
    line_3:        evolution of intermediate mass stars, it is proposed to use the WF/PC to look
    line_4:        for evidence of evaporation of massive comets by the strong stellar wind and
    line_5:        radiation field of these stars.

!
! end of abstract

general_form_proposers:

  lname:           O'DELL
    fname:         C.
    mi:            R.
    inst:          RICE UNIVERSITY
    country:       USA

!

  lname:           SPITZER JR.
    fname:         LYMAN
    inst:          PRINCETON UNIVERSITY
    country:       USA

!
! end of general_form_proposers block

general_form_text:

  question:        3
    section:       1
    line_1:        Images will be made with a Ly alpha (F122M) and OH (F284W) filters of the WF/PC
    line_2:        in the WF mode for NGC 3587 and 7293.

!

  question:        4
    section:       1
    line_1:        Only HST allows the high angular resolution necessary for this program.

!

  question:        7
    section:       1
    line_1:        Images will be standard processed at the STScI, then submitted to enhancement
    line_2:        and analysis with the Rice University Image Processing Facility.

!

  question:        10
    section:       1
    line_1:        The principal resources at Rice University are the Image Processing Facility
    line_2:        and availability of graduate student assistants.

!

  question:        13
    section:       1
    line_1:        Under the assumptions that the Oort Cloud of Comets is a common feature of
    line_2:        stars with planetary systems and that planetary nebulae nuclei are advanced
    line_3:        stages of evolution of intermediate mass stars, it is proposed to use the WF/PC
    line_4:        to look for evidence of evaporation of massive comets by the strong stellar
    line_5:        wind and radiation field of these stars.

!
!end of general form text

general_form_address:

  lname:           SPITZER JR.
    fname:         LYMAN
    inst:          PRINCETON UNIVERSITY OBSERVATORY
    addr_1:        PEYTON HALL
    city:          PRINCETON
    state:         NJ
    zip:           08544
    country:       USA
    phone:         (609) 452-3809

!

  lname:           O'DELL
    fname:         C.
    mi:            R.
    title:         PROF.
    category:      PI
    inst:          RICE UNIVERSITY
    addr_1:        DEPT. OF SPACE PHYSICS & ASTRONOMY
    addr_2:        P.O. BOX 1892
    city:          HOUSTON
    state:         TX
    zip:           77251
    country:       USA
    phone:         713-527-8101 X3633
    telex:         556457

!
! end of general_form_address records

fixed_targets:

    targnum:       1
    name_1:        PK36-57D1
    name_2:        HELIX-NEBULA
    descr_1:       G,502
    pos_1:         RA = 22H 26M 55S +/- 1S,
    pos_2:         DEC = -21D 03' 05" +/- 20"
    equinox:       1950
    fluxnum_1:     1
    fluxval_1:     SURF-LINE(4861)=1.2+/-0.1E-15,
    fluxval_2:     W-LINE(4861)=1+/-0

!

    targnum:       2
    name_1:        PK148+57D1
    name_2:        OWL-NEBULA
    descr_1:       G,502
    pos_1:         RA = 11H 09M 00.3S +/- 1S,
    pos_2:         DEC = +55D 33' 45" +/- 10"
    equinox:       1900
    fluxnum_1:     1
    fluxval_1:     SURF-LINE(4861)=1.2+/-0.1E-15,
    fluxval_2:     W-LINE(4861)=1+/-0

!
! end of fixed targets

! No solar system records found

! No generic target records found

exposure_logsheet:

    linenum:       1.000
    targname:      PK36-57D1
    config:        WFC
    opmode:        IMAGE
    aperture:      ALL
    sp_element:    F122M
    num_exp:       1
    time_per_exp:  40M
    s_to_n:        20
    fluxnum_1:     1
    priority:      1
    param_1:       SUM=2X2
    req_1:         CYCLE 9 / 1-4

!

    linenum:       2.000
    targname:      PK36-57D1
    config:        WFC
    opmode:        IMAGE
    aperture:      ALL
    sp_element:    F284W
    num_exp:       1
    time_per_exp:  40M
    s_to_n:        10
    fluxnum_1:     1
    priority:      1
    param_1:       SUM=2X2

!

    linenum:       3.000
    targname:      PK148+57D1
    config:        WFC
    opmode:        IMAGE
    aperture:      ALL
    sp_element:    F122M
    num_exp:       1
    time_per_exp:  40M
    s_to_n:        20
    fluxnum_1:     1
    priority:      1
    param_1:       SUM=2X2

!

    linenum:       4.000
    targname:      PK148+57D1
    config:        WFC
    opmode:        IMAGE
    aperture:      ALL
    sp_element:    F284W
    num_exp:       1
    time_per_exp:  40M
    s_to_n:        10
    fluxnum_1:     1
    priority:      1
    param_1:       SUM=2X2

!
! end of exposure logsheet

! No scan data records found