! File: 3338C.PROP ! Database: PEPDB ! Date: 19-FEB-1994:03:56:28 coverpage: title_1: STAR FORMATION REGIONS: HH AND T TAU OBJECTS sci_cat: INTERSTELLAR MEDIUM sci_subcat: HH OBJECTS proposal_for: GTO/FOC pi_fname: J. CHRIS pi_lname: BLADES pi_inst: ESA, SPACE TELESCOPE SCIENCE INSTITUTE pi_country: USA pi_phone: (301)338-4805 keywords_1: STAR FORMATION - INTERSTELLAR MEDIUM - HH OBJECTS - keywords_2: TTAU OBJECTS hours_pri: 19.20 num_pri: 12 realtime: X pi_position: DR. J. C. BLADES ! end of coverpage abstract: line_1: It is proposed to study objects in their early stages of formation to line_2: investigate the intrinsic properties of these young objects and to establish line_3: the nature of their interaction with the local ISM. Time variablity of these line_4: targets is an important parameter, the targets will be revisited several times line_5: during the GTO phase. line_7: The program requires both the high-resolution, ultraviolet imaging and the line_8: long-slit spectrograph of the FOC for its success. ! ! end of abstract general_form_proposers: lname: BLADES fname: J. CHRIS inst: ESA, SPACE TELESCOPE SCIENCE INSTITUTE country: USA esa: X ! ! end of general_form_proposers block general_form_text: question: 12 section: 1 line_1: Several targets will be revisited during the GTO period, the purpose being line_2: to study their temporal variation which is expected to give an insight into line_3: their physical nature. Hence, it would be premature, and would certainly line_4: compromise the scientific goals of the program, if their data were released line_5: before one year had elapsed after the final observation. ! question: 13 section: 1 line_1: It is proposed to study objects in their early stages of star to line_2: investigate the intrinsic properties of these young objects and to establish line_3: the nature of their interaction with the local ISM. Time variability to these line_4: targets is an important parameter, the targets will be revisited several times line_5: durng the GTO phase. line_7: Several targets will be revisited during the GTO period, the purpose being to line_8: study their temporal variation which is expected to give an insight into their line_9: physical nature. Hence, it would be premature, and would certainly compromise line_10: the scientific goals of the program, if the early data were released before one line_11: year had elapsed after the final observation. ! !end of general form text general_form_address: lname: BLADES fname: J. CHRIS category: PI inst: ESA, SPACE TELESCOPE SCIENCE INSTITUTE ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: HH1 descr_1: SEMI-STELLAR KNOTS, pos_1: RA = 05H 36M 20.451S +/- 0.02S, pos_2: DEC = -06D 45' 10.72" +/- 0.3", pos_3: PLATE-ID = 02NB equinox: 2000 pm_or_par: N ! targnum: 2 name_1: HH2 descr_1: SEMI-STELLAR KNOTS pos_1: RA = 05H 36M 25.51S +/- 0.02S, pos_2: DEC = -06D 47' 11.58" +/-0.3", pos_3: PLATE-ID = 02NB equinox: 2000 pm_or_par: N ! targnum: 3 name_1: HH-CS descr_1: CENTRAL STAR pos_1: RA = 05H 33M 55.55S +/- 0.2S, pos_2: DEC = -06D 47' 25.1" +/- 3" equinox: 1950 pm_or_par: ^ ! targnum: 4 name_1: HH30 descr_1: REFLECTION NEBULA pos_1: RA = 04H 28M 43S +/- 0.2S, pos_2: DEC = +25D 57' 43" +/- 3" equinox: ^ pm_or_par: ^ ! targnum: 5 name_1: DG-TAU-B descr_1: T TAURI STAR pos_1: RA = 04H 24M 07.6S +/- 0.2S, pos_2: DEC = +25D 58' 48" +/- 3" equinox: ^ pm_or_par: ^ fluxnum_1: 1 fluxval_1: V = 20.5 ! targnum: 6 name_1: IRS5 descr_1: INFRARED SOURCE pos_1: RA = 04H 28M 39.7S +/- 0.2S, pos_2: DEC = +18D 01' 45" +/- 3" equinox: ^ pm_or_par: ^ ! targnum: 7 name_1: T-TAU descr_1: T TAURI STAR pos_1: RA = 04H 19M 04S +/- 0.2S, pos_2: DEC = +19D 25' 04" +/- 3" equinox: ^ pm_or_par: ^ fluxnum_1: 1 fluxval_1: U = 11 fluxnum_2: 2 fluxval_2: F-LINE (2800) = 5.4 E-12 fluxnum_3: 3 fluxval_3: F-LINE (1549) = 2 E-13 ! targnum: 8 name_1: DG-TAU descr_1: ^ pos_1: RA = 04H 24M 00.6S +/- 0.2S, pos_2: DEC = +25D 59' 35" +/- 3" equinox: ^ pm_or_par: ^ fluxnum_1: 1 fluxval_1: U = 12 fluxnum_2: 2 fluxval_2: F-LINE (2800) = 1.2 E-12 ! targnum: 9 name_1: HL-TAU descr_1: ^ pos_1: RA = 04H 28M 44.1S +/- 0.2S, pos_2: DEC = +18D 07' 37" +/- 3" equinox: ^ pm_or_par: ^ fluxnum_1: 1 fluxval_1: U = 14.7 ! targnum: 10 name_1: XZ-TAU descr_1: T TAURI STAR pos_1: RA = 04H 28M 45.7S +/- 0.2S, pos_2: DEC = +18D 07' 35" +/- 3" equinox: 1950 pm_or_par: N fluxnum_1: 1 fluxval_1: U = 14.6 ! targnum: 11 name_1: RW-AUR descr_1: ^ pos_1: RA = 05H 04M 37.3S +/- 0.2S, pos_2: DEC = +30D 20' 13" +/- 3" equinox: ^ pm_or_par: ^ fluxnum_1: 1 fluxval_1: U = 11 fluxnum_2: 2 fluxval_2: F-LINE (2800) = 1.6 E-11 fluxnum_3: 3 fluxval_3: F-LINE (1549) = 1.2 E-13 ! targnum: 12 name_1: RU-LUPI descr_1: T TAURI STAR pos_1: RA = 15H 53M 22.9S +/- 0.2S, pos_2: DEC = -37D 40' 58" +/- 3" equinox: 1950 pm_or_par: N fluxnum_1: 1 fluxval_1: U = 11 fluxnum_2: 2 fluxval_2: F-LINE (2800) = 1.5 E-12 fluxnum_3: 3 fluxval_3: F-LINE (1549) = 1.5 E-12 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 3.000 sequence_1: DEFINE sequence_2: RUN1 targname: # config: FOC/96 opmode: IMAGE aperture: 512X512 sp_element: F501N num_exp: 2 time_per_exp: 1000S priority: # ! linenum: 3.010 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F372M num_exp: 2 time_per_exp: 1000S priority: # ! linenum: 3.015 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F486N num_exp: 2 time_per_exp: 1000S priority: # ! linenum: 3.020 sequence_1: DEFINE sequence_2: RUN2 targname: # config: FOC/96 opmode: IMAGE aperture: 512X1024 sp_element: F501N num_exp: 1 time_per_exp: 1500S priority: # ! linenum: 3.025 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F372M num_exp: 1 time_per_exp: 1500S priority: # ! linenum: 3.030 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F486N num_exp: 1 time_per_exp: 1500S priority: # ! linenum: 3.040 sequence_1: DEFINE sequence_2: RUN3 targname: # config: FOC/96 opmode: IMAGE aperture: 512X512 sp_element: F501N num_exp: 1 time_per_exp: 900S priority: # req_1: CYCLE 2; req_2: COND IF TAC OK; req_3: GUID TOL 0.020"; ! linenum: 3.200 sequence_1: USE sequence_2: RUN1 targname: HH1 priority: 1 req_1: CYCLE 2; req_2: GUID TOL 0.020" / 3.2-3.5; ! linenum: 3.300 sequence_1: USE sequence_2: RUN2 targname: HH2 priority: 1 req_1: CYCLE 2; ! linenum: 3.400 sequence_1: USE sequence_2: RUN1 targname: HH1 priority: 1 req_1: CYCLE 9; ! linenum: 3.500 sequence_1: USE sequence_2: RUN2 targname: HH2 priority: 1 req_1: CYCLE 9; ! linenum: 4.000 sequence_1: USE sequence_2: RUN3 targname: HH30 priority: 1 ! linenum: 5.000 sequence_1: USE sequence_2: RUN3 targname: DG-TAU-B priority: 1 ! linenum: 6.000 sequence_1: USE sequence_2: RUN3 targname: IRS5 priority: 1 ! linenum: 7.000 sequence_1: USE sequence_2: RUN3 targname: RU-LUPI priority: 1 ! linenum: 8.000 sequence_1: USE sequence_2: RUN3 targname: HL-TAU priority: 1 ! linenum: 9.000 sequence_1: USE sequence_2: RUN3 targname: T-TAU priority: 1 ! linenum: 10.000 sequence_1: USE sequence_2: RUN3 targname: RW-AUR priority: 1 ! linenum: 11.000 sequence_1: USE sequence_2: RUN3 targname: DG-TAU priority: 1 ! linenum: 12.000 sequence_1: USE sequence_2: RUN3 targname: XZ-TAU priority: 1 ! ! end of exposure logsheet ! No scan data records found