!  File:  4841C.PROP
!  Database:  PEPDB
!  Date:  23-FEB-1994:05:44:41

coverpage:

  title_1:         DQ HER-FOS SPECTRA:CYC3MEDIUM
    sci_cat:       STELLAR ASTROPHYSICS
    sci_subcat:    SUBLUMINOUS STARS
    proposal_for:  GTO/OS
    cont_id:       1067
    pi_title:      PROF.
    pi_fname:      DAVID
    pi_mi:         L.
    pi_lname:      LAMBERT
    pi_inst:       TEXAS, UNIVERSITY OF
    pi_country:    USA
    pi_phone:      512-471-7438
    keywords_1:    VARIABLE STARS: NOVAE
    keywords_2:    INDIVIDUAL: DQ HER
    hours_pri:     2.62
    num_pri:       2
    fos:           X
    pi_position:   PROFESSOR
! end of coverpage

abstract:

    line_1:        The classical nova DQ Her is the prototype of the dust-forming novae with the
    line_2:        1934 ejecta well resolved on the sky providing an emission line spectrum
    line_3:        corresponding to an electron temperature of just T ~ 500K.
    line_4:        FOS spectra will be obtained of knots in the nebula.

!
! end of abstract

general_form_proposers:

  lname:           LAMBERT
    fname:         DAVID
    mi:            L.
    inst:          TEXAS, UNIVERSITY OF
    country:       USA

!

  lname:           FERLAND
    fname:         GARY
    mi:            J.
    inst:          KENTUCKY, UNIVERSITY OF
    country:       USA

!
! end of general_form_proposers block

general_form_text:

  question:        3
    section:       1
    line_1:        FOS G160L spectra will be obtained of 2 knots in the DQ Her
    line_2:        nebula. The knots will be identified froma WFC image to be
    line_3:        obtained as an early acquisition exposure,
    line_4:        as well as a scientific image.

!

  question:        4
    section:       1
    line_1:        The ultraviolet is essential for key lines and the scattered continuum
    line_2:        contributed by the higher scattering cross-section of dust grains in DQ Her's
    line_3:        nebula. HST also provides the higher spatial resolution needed to resolve fine
    line_4:        filamentary structure.

!

  question:        7
    section:       1
    line_1:        Spectra as reduced by the standard STScI software will be analyzed at the
    line_2:        University of Texas. WF/PC images will probably be handled at STScI.
    line_4:        Interpretation will be integrated with our present work on DQ Her and related
    line_5:        old novae.

!

  question:        10
    section:       1
    line_1:        University and Departmental computing facilities.

!

  question:        13
    section:       1
    line_1:        Ultraviolet spectra and images of the DQ Her's nebula will provide information
    line_2:        on the gas and dust content of the cool ejecta from the 1934 outburst.

!
!end of general form text

general_form_address:

  lname:           LAMBERT
    fname:         DAVID
    mi:            L.
    title:         PROF.
    category:      PI
    inst:          UNIVERSITY OF TEXAS
    addr_1:        ASTRONOMY DEPARTMENT
    addr_2:        RLM 15.308
    city:          AUSTIN
    state:         TX
    zip:           78712
    country:       USA
    phone:         512-471-7438
    telex:         910-874-1351

!
! end of general_form_address records

fixed_targets:

    targnum:       1
    name_1:        DQ-HER
    descr_1:       A,152,161,917
    pos_1:         RA = 18H 06M 5.3S +/- .5S,
    pos_2:         DEC = +45D 51' 01" +/- 2"
    equinox:       1950
    pm_or_par:     N
    fluxnum_1:     1
    fluxval_1:     V=14.2
    fluxnum_2:     2
    fluxval_2:     SURF(6563)=4 +/- 2 E-16
    fluxnum_3:     3
    fluxval_3:     W-LINE(6563)=1.0 +/- 0.2

!

    targnum:       2
    name_1:        DQ-HER-A
    descr_1:       A,152,161,917
    pos_2:         RA-OFF=-0.6S +/- 0.3S,
    pos_3:         DEC-OFF= 8" +/- 4",
    pos_4:         FROM 1
    equinox:       1950
    pm_or_par:     N
    comment_1:     TBD-EARLY FROM A WFC IMAGE TAKEN
    comment_2:     IN A RELATED PROPOSAL
    comment_3:     POSITION 2 CORRESPONDS TO LOCATION
    comment_4:     A OF WILLIAMS ET AL. APJ 224 171
    comment_5:     1978

!

    targnum:       3
    name_1:        DQ-HER-B
    descr_1:       A,152,161,917
    pos_2:         RA-OFF=+0.6S +/- 0.3S,
    pos_3:         DEC-OFF= +5" +/- 2",
    pos_4:         FROM 1
    equinox:       1950
    pm_or_par:     N
    comment_1:     TBD-EARLY FROM A WFC IMAGE TAKEN
    comment_2:     IN A RELATED PROPOSAL
    comment_3:     POSITION 3 CORRESPONDS TO LOCATION
    comment_4:     B OF WILLIAMS ET AL. APJ 224 171
    comment_5:     1978

!
! end of fixed targets

! No solar system records found

! No generic target records found

exposure_logsheet:

    linenum:       1.000
    targname:      DQ-HER
    config:        FOS/BL
    opmode:        ACQ/BINARY
    aperture:      4.3
    sp_element:    MIRROR
    num_exp:       1
    time_per_exp:  5S
    fluxnum_1:     1
    priority:      2
    req_1:         SEQ 1-3 NO GAP;
    req_2:         ONBOARD ACQ FOR 2-3;
    req_3:         CYCLE 3 / 1-3
    comment_1:     SMALLER APERTURE MAY BE USED
    comment_2:     FOR 1-3 IF WFC IMAGE SHOWS
    comment_3:     VERY SMALL KNOTS

!

    linenum:       2.000
    targname:      DQ-HER-A
    config:        FOS/BL
    opmode:        ACCUM
    aperture:      4.3
    sp_element:    G160L
    wavelength:    1150-2524
    num_exp:       1
    time_per_exp:  40M
    priority:      2

!

    linenum:       3.000
    targname:      DQ-HER-B
    config:        FOS/BL
    opmode:        ACCUM
    aperture:      4.3
    sp_element:    G160L
    wavelength:    1150-2524
    num_exp:       1
    time_per_exp:  40M
    priority:      2

!
! end of exposure logsheet

! No scan data records found