! File: 1150C.PROP ! Database: PEPDB ! Date: 16-FEB-1994:03:41:50 coverpage: title_1: STELLAR WINDS IN M31, M33 sci_cat: STELLAR ASTROPHYSICS sci_subcat: HOT STARS proposal_for: GTO/HRS pi_title: PROF. pi_fname: JOHN pi_mi: B. pi_lname: HUTCHINGS pi_inst: DOMINION ASTROPHYSICAL OBSERVATORY pi_country: CANADA pi_phone: (604) 388-3909 keywords_1: HOT STARS, MASS-LOSS, STELLAR WINDS hours_pri: 2.00 num_pri: 8 pi_position: PROFESSOR ! end of coverpage abstract: line_1: We will obtain UV spectra of OB supergiant stars in M33 AND M31 to study line_2: stellar wind phenomena (resonance line profiles and velocities, stellar line_3: effective temperatures). We will also derive approximate UV extinction curves line_4: for these galaxies. These observations relate to global comparisons between line_5: galaxies of different types. WFC UV grating images are requested in parallel line_6: to study the OB star population and extinction in these galaxies. ! ! end of abstract general_form_proposers: lname: MASSEY fname: P. inst: NOAO, KITT PEAK NATIONAL OBSERVATORY country: USA ! lname: HUTCHINGS fname: JOHN mi: B. inst: DOMINION ASTROPHYSICAL OBSERVATORY country: CANADA ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: FOS UV spectra will be taken in the range Lambda-Lambda line_2: 1100-3000, to derive line profiles and flux distributions, of several selected line_3: OB stars. The stars are selected on the basis of ground-based spectroscopy and line_4: in some cases, low dispersion IUE spectra. line_5: Parallel WFC images with the UV grating G200L are requested in all fields. ! question: 4 section: 1 line_1: Only HST can obtain UV spectra with the desired resolution and S/N. ! question: 7 section: 1 line_1: Spectra will be analysed using DAO and KPNO facilities. Stellar effective line_2: temperatures, fluxes and extinction will be estimated by comparison with model line_3: atmospheres, line profiles and velocities will be compared with galactic and MC line_4: counterparts. ! question: 8 section: 1 line_1: Targets and/or positions may be updated if ground-based research progress line_2: warrants it. ! question: 10 section: 1 line_1: All resources supplied by DAO and KPNO. ! question: 13 section: 1 line_1: Comparative stellar wind studies will be made between M31 and m33 OB line_2: stars. Obsevations are UV spectra of 2-3 stars from each line_3: galaxy, selected from ground-based spectroscopy. ! !end of general form text general_form_address: lname: HUTCHINGS fname: JOHN mi: B. title: PROF. category: PI inst: DOMINION ASTROPHYSICAL OBSERVATORY addr_1: 5071 W. SAANICH RD. addr_2: V8X 4M6 city: VICTORIA state: BC country: CANADA phone: (604) 363-0018 telex: 049-7295 ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: OB48/527 descr_1: OB STAR IN M31 pos_1: RA=0H 42M 32.595S+/-1", pos_2: DEC=41D 22' 58.32"+/-1" equinox: 1950 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 1.000 targname: OB48/527 config: FOS/BL opmode: ACQ/BINARY aperture: 4.3 sp_element: MIRROR num_exp: 1 time_per_exp: 60S priority: 1 req_1: ONBOARD ACQ FOR 2-4; req_2: CYCLE 1 /1-4 ! linenum: 2.000 targname: ^ config: ^ opmode: ACCUM aperture: 1.0 sp_element: G130H wavelength: 1150-1608 num_exp: 1 time_per_exp: 3200S priority: 1 req_1: UNPROTECTED ! linenum: 3.000 targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: G190H wavelength: 1595-2282 num_exp: ^ time_per_exp: 1200S priority: ^ req_1: UNPROTECTED ! linenum: 4.000 targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: G270H wavelength: 2227-3306 num_exp: ^ time_per_exp: 350S priority: ^ req_1: UNPROTECTED ! ! end of exposure logsheet ! No scan data records found