! File: 3196C.PROP ! Database: PEPDB ! Date: 18-FEB-1994:21:34:27 coverpage: title_1: IMAGING AND UV SPECTROPHOTOMETRY OF LOCAL GROUP PLANETARY NEBULAE title_2: (FOS 26): CYCLE 1 OBSERVATIONS sci_cat: INTERSTELLAR MEDIUM proposal_for: GTO/FOS cont_id: 1046 pi_title: DR. pi_fname: HOLLAND pi_mi: C. pi_lname: FORD pi_inst: SPACE TELESCOPE SCIENCE INSTITUTE pi_country: USA pi_phone: (301) 338-4803 keywords_1: NEBULA, PLANETARIES, CENTRAL STARS, GALAXIES, K648 hours_pri: 2.40 num_pri: 2 fos: Y ! end of coverpage abstract: line_1: WF/PC interference filter pictures will be used to resolve the shells of line_2: planetary nebulae in the LMC and to resolve the shell of K648 in M15. The line_3: angular diameters of the shells will be combined with echelle expansion line_4: velocities to derive the ages of nebulae. Ultraviolet spectra of the central line_5: stars will be used to derive the stars' effective temperatures and magnitudes, line_6: with objective of placing the stars on evolutionary tracks in an M-Teff line_7: diagram. UV spectra of the LMC nebulae, K648, and the brightest nebula in M32, line_8: NGC205, and NGC185 will be used to derive chemical compositions and physical line_9: conditions in the nebulae. ! ! end of abstract general_form_proposers: lname: BEAVER fname: EDWARD inst: UC, SAN DIEGO country: USA ! lname: BURBIDGE fname: E. MARGARET inst: UC, SAN DIEGO country: USA ! lname: MARGON fname: BRUCE inst: WASHINGTON, UNIVERSITY OF country: USA ! lname: ANGEL fname: J. ROGER mi: P. inst: ARIZONA, UNIVERSITY OF country: USA ! lname: BARTKO fname: FRANK inst: APPLIED RESEARCH CORPORATION country: USA ! lname: DAVIDSEN fname: ARTHUR mi: F. inst: JOHNS HOPKINS UNIVERSITY country: USA ! lname: HARMS fname: RICHARD mi: J. inst: APPLIED RESEARCH CORPORATION country: USA ! lname: BOHLIN fname: RALPH inst: SPACE TELESCOPE SCIENCE INSTITUTE country: USA ! lname: FORD fname: HOLLAND mi: C. inst: SPACE TELESCOPE SCIENCE INSTITUTE country: USA ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: Cycle 1: 101-104 ! question: 5 section: 1 line_1: ! question: 5 section: 2 line_1: The SV prerequisite programs for all FOS line_2: observations in this program are: line_3: Prop ID 2195 FOS Target Acquisition Tests line_4: - All observations line_5: Prop ID 1317 Int./Ext. Wavelength Offsets line_6: - 1st target line_7: Prop ID 1318 Spectral Flat Fields line_8: - 1st target line_9: Prop ID 1320 Absolute Spectrophotometry line_10: - 1st visit of bright targets line_11: All WF/PC imaging with a center wavelength line_12: blueward of 5000 Angstroms requires UV flood ! question: 12 section: 1 line_1: The observations of the LMC planetaries constitute an integrated program to line_2: establish to evolution of central stars, and will not be complete until seven line_3: of the nine have been observed. Data should not be released until one year line_4: after completion of the seventh planetary nebula. Likewise, the three line_5: planetaries in NGC205, NGC185, and M32 constitute a program which will not be line_6: complete until two of the three planetaries have been observed. ! question: 13 section: 1 line_1: WF/PC pictures of K648 and LMC planetaries will be used to resolve their line_2: shells. Small aperture FOS UV spectra of the central stars will be used to line_3: place the central stars on evolutionary tracks in an M-Teff diagram. Chemical line_4: composition and physical conditions in the shells will be derived from UV line_5: spectra of the nebulae. ! !end of general form text general_form_address: lname: FORD fname: HOLLAND mi: C. title: DR. category: PI inst: SPACE TELESCOPE SCIENCE INSTITUTE addr_1: HOMEWOOD CAMPUS addr_2: 3700 SAN MARTIN DRIVE city: BALTIMORE state: MD zip: 21218 country: USA phone: (301) 338-4803 ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: K648 descr_1: G,502 pos_1: RA=21H 29M 59.4175S +/- 0.3", pos_2: DEC=+12D 10' 25.987" +/- 0.3", pos_3: PLATE-ID=02V2 equinox: 2000 rv_or_z: V=-115 fluxnum_1: 1 fluxval_1: F-LINE(5007)=1.5E-12, E(B-V)=0.08 ! targnum: 2 name_1: K648-OFFSET descr_1: A,140 pos_1: RA-OFF=+0.9375S +/- 0.0014S, pos_2: DEC-OFF=+24.553" +/- 0.02", pos_3: FROM 1 equinox: 2000 fluxnum_1: 1 fluxval_1: V=12.98 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 101.000 targname: K648-OFFSET config: FOS/BL opmode: ACQ/BINARY aperture: 4.3 sp_element: MIRROR num_exp: 1 time_per_exp: 9.0S priority: 1 req_1: ONBOARD ACQ FOR 101.5-104; req_2: GROUP 101-104 WITHIN 15D; req_3: CYCLE 2 / 101-104 ! linenum: 101.500 targname: K648 config: FOS/BL opmode: ACQ aperture: 4.3 sp_element: MIRROR num_exp: 1 time_per_exp: 63S priority: 1 ! linenum: 102.000 targname: K648 config: FOS/BL opmode: ACCUM aperture: 1.0 sp_element: G270H num_exp: 1 time_per_exp: 600S priority: 1 ! linenum: 103.000 targname: K648 config: FOS/BL opmode: ACCUM aperture: 1.0 sp_element: G190H num_exp: 1 time_per_exp: 900S priority: 1 ! linenum: 104.000 targname: K648 config: FOS/BL opmode: ACCUM aperture: 1.0 sp_element: G130H num_exp: 1 time_per_exp: 3600S priority: 1 ! ! end of exposure logsheet ! No scan data records found