! Proposal 5883, submission 1 ! PI: Francis Keenan ! Received Mon Feb 13 09:43:25 EST 1995 ! From: sembach@sundoggie.mit.edu ! Revised 6/28/95 Proposal_Information Title: Properties of the High-Velocity Cloud Towards HD 203664 Proposal_Category: GO Scientific_Category: Interstellar Medium Cycle: 5 Investigators PI_name: Francis Keenan PI_Institution: The Queen's University of Belfast CoI_Name: Philip Dufton CoI_Institution: The Queen's University of Belfast Contact: N CoI_Name: Kenneth Sembach CoI_Institution: Massachusetts Institute of Technology Contact: Y Abstract: We will obtain high- and intermediate-resolution GHRS spectra of the +70 km/sec HVC seen toward HD 203664 in optical and radio spectra. The observations will provide a unique opportunity to quantify the ionization structure of a HVC and accurately determine the chemical abundances of important elements such as C, N, O, Mg, Si, S, Cr, Mn, Fe, and Zn in high velocity interstellar material. Our high spectral resolution optical data suggest that substructure may exist within the HVC which, if confirmed, would support the possibility that early-type stars at large distances from the Galactic plane are formed through star formation induced by collisions between cloudlets within HVCs. We will test this hypothesis on the HD 203664 HVC with high S/N absorption line measurements made by the GHRS in its highest resolution mode. By combining a supporting set of optical and radio data with the ultraviolet observations, we will study the velocity structure of the HVC, morphology, distance, and physical conditions of this HVC in greater detail than has been possible for any other high velocity cloud in the sky. Questions Observing_Description: We will obtain spectroscopic observations of the HVC absorption toward HD 203664 using both the highest resolution (echelle) and intermediate resolution gratings of the GHRS. The light of HD 203664 will be placed in the large science aperture (LSA). The data will be obtained with the default diode substepping (step-patterns 5 and 7). Comb-addition and the FP-SPLIT=4 procedures will be used to reduce fixed pattern noise in the data. All exposures will be broken into shorter exposures (either through the use of FP-SPLIT or through explicit breaks) to ensure that geomagnetically-induced image blurring of the data is minimized. Resolution and sensitivity estimates were taken from the post-COSTAR GHRS instrument handbook (Version 5.0, May 1994). Flux estimates for each observation were determined from our recent IUE echelle spectra and should be accurate to ~15%. Exposure calculations include an allowance for background determinations with the full diode array as part of the substepping procedures. The expected S/N values of ~50-70 are appropriate for a (Nyquist) sampling of 2 substeps/diode, but we will obtain 4 samples per diode and rebin the data without loss of resolution after acquisition. Real_Time_Justification: No special scheduling requirements are necessary. Calibration_Justification: No special scheduling requirements are necessary. Additional_Comments: No additional comments at this time. Fixed_Targets ! Section 5.1 Target_Number: 1 Target_Name: HD203664 Alternate_Names: BD+09D4793, GSC1110-01376 Description: STAR, B0-B2 V-IV Position: RA=21H 23M 28.84S +/- 0.02S, DEC=+09D 55' 54.7" +/- 0.3" Equinox: J2000 RV_or_Z: V = +110 RA_PM: +0.0003 Dec_PM: -0.014 Epoch: 2000.000 Annual_Parallax: Flux: V = 8.42 +/- 0.40, B-V = -0.19 +/- 0.10, F-CONT(1240) = 4.0 +/- 0.2 E-11, F-CONT(1550) = 0.8 +/- 0.2 E-11, F-CONT(2600) = 1.1 +/- 0.2 E-11 Comments: Hipparcos coords and proper motions. Visits !Visit Number 1 Visit_Number: 1 Visit_Requirements: On_Hold_Comments: Visit_Comments: First visit to obtain Side 1 spectra (4 orbits). Number exposures beginning with 10. !Line 1 Exposure_Number: 10 Target_Name: HD203664 Config: HRS Opmode: ACQ Aperture: 2.0 Sp_Element: MIRROR-N1 Wavelength: Optional_Parameters: BRIGHT=RETURN, SEARCH-SIZE=3 Number_of_Iterations: 1 Time_Per_Exposure: 1.8S Special_Requirements: ONBOARD ACQ FOR 20-70 Comments: Expect about 74,000 cnt/s using mirror N1. STEP-TIME = 0.2 seconds. Ok as long as BRIGHT=RETURN is used. !Line 2 Exposure_Number: 20 Target_Name: HD203664 Config: HRS Opmode: ACCUM Aperture: 2.0 Sp_Element: ECH-A Wavelength: 1335.1 Optional_Parameters: FP-SPLIT=FOUR, COMB=FOUR, STEP-PATT=7, DOPPLER=ON Number_of_Iterations: 1 Time_Per_Exposure: 1523.2S !(S/N=50 @ 25.8M) Special_Requirements: Comments: Lines = C II, C II* !Line 3 Exposure_Number: 30 Target_Name: HD203664 Config: HRS Opmode: ACCUM Aperture: 2.0 Sp_Element: ECH-A Wavelength: 1303.4 Optional_Parameters: FP-SPLIT=FOUR, COMB=FOUR, STEP-PATT=7, DOPPLER=ON Number_of_Iterations: 1 Time_Per_Exposure: 1305.6S !(S/N=50 @ 21.2M) Special_Requirements: Comments: Lines = O I, O I*, Si II, S I !Line 4 Exposure_Number: 40 Target_Name: HD203664 Config: HRS Opmode: ACCUM Aperture: 2.0 Sp_Element: G140M Wavelength: 1396.5 Optional_Parameters: FP-SPLIT=FOUR, COMB=FOUR, STEP-PATT=5, DOPPLER=ON Number_of_Iterations: 1 ! Time_Per_Exposure: 979.2S !(S/N=50 @ 17.0M) Time_Per_Exposure: 1196.8S !(S/N=50 @ 17.0M) Special_Requirements: Comments: Lines = Si IV, Ni II !Line 5 Exposure_Number: 50 Target_Name: HD203664 Config: HRS Opmode: ACCUM Aperture: 2.0 Sp_Element: G140M Wavelength: 1248.3 Optional_Parameters: FP-SPLIT=FOUR, COMB=FOUR, STEP-PATT=5, DOPPLER=ON Number_of_Iterations: 1 ! Time_Per_Exposure: 652.8S !(S/N=70 @ 10.6M) Time_Per_Exposure: 761.6S !(S/N=70 @ 10.6M) Special_Requirements: Comments: Lines = Ge II, N V, Mg II, S I, S II, Si II !Line 6 Exposure_Number: 60 Target_Name: HD203664 Config: HRS Opmode: ACCUM Aperture: 2.0 Sp_Element: G140M Wavelength: 1544.5 Optional_Parameters: FP-SPLIT=FOUR, COMB=FOUR, STEP-PATT=5, DOPPLER=ON Number_of_Iterations: 2 Time_Per_Exposure: 1523.2S !(S/N=50 @ 27.1M) Special_Requirements: Comments: Lines = P II, C IV !Line 7 Exposure_Number: 70 Target_Name: HD203664 Config: HRS Opmode: ACCUM Aperture: 2.0 Sp_Element: G140M Wavelength: 1199.0 Optional_Parameters: FP-SPLIT=FOUR, COMB=FOUR, STEP-PATT=5, DOPPLER=ON Number_of_Iterations: 1 Time_Per_Exposure: 1305.6S !(S/N=50 @ 19.5M) Special_Requirements: Comments: Lines = S III, Si II, Si III, Mn II, N I !Visit Number 2 Visit_Number: 2 Visit_Requirements: On_Hold_Comments: Visit_Comments: Second visit to obtain Side 2 spectra (5 orbits). Number exposures beginning with 110. !Line 11 Exposure_Number: 110 Target_Name: HD203664 Config: HRS Opmode: ACQ Aperture: 2.0 Sp_Element: MIRROR-N2 Wavelength: Optional_Parameters: BRIGHT=RETURN, SEARCH-SIZE=3 Number_of_Iterations: 1 Time_Per_Exposure: 1.8S Special_Requirements: ONBOARD ACQ FOR 120-210 Comments: Expect about 400,000 cnt/s using mirror N2. STEP-TIME = 0.2 seconds. Ok as long as BRIGHT=RETURN is used. !Line 12 Exposure_Number: 120 Target_Name: HD203664 Config: HRS Opmode: ACCUM Aperture: 2.0 Sp_Element: ECH-B Wavelength: 2061.62 Optional_Parameters: FP-SPLIT=FOUR, COMB=FOUR, STEP-PATT=7, DOPPLER=ON Number_of_Iterations: 2 Time_Per_Exposure: 761.6S !(S/N=50 @ 24.6M) Special_Requirements: Comments: Lines = Cr II, Zn II !Line 13 Exposure_Number: 130 Target_Name: HD203664 Config: HRS Opmode: ACCUM Aperture: 2.0 Sp_Element: ECH-B Wavelength: 1807.6 Optional_Parameters: FP-SPLIT=FOUR, COMB=FOUR, STEP-PATT=7, DOPPLER=ON Number_of_Iterations: 2 Time_Per_Exposure: 979.2S !(S/N=50 @ 37.6M) Special_Requirements: Comments: Lines = Si II, S I, Ni II !Line 14 Exposure_Number: 140 Target_Name: HD203664 Config: HRS Opmode: ACCUM Aperture: 2.0 Sp_Element: ECH-B Wavelength: 2371.3 Optional_Parameters: FP-SPLIT=FOUR, COMB=FOUR, STEP-PATT=7, DOPPLER=ON Number_of_Iterations: 1 Time_Per_Exposure: 761.6S !(S/N=50 @ 11.4M) Special_Requirements: Comments: Lines = Fe II !Line 15 Exposure_Number: 150 Target_Name: HD203664 Config: HRS Opmode: ACCUM Aperture: 2.0 Sp_Element: ECH-B Wavelength: 2603.3 Optional_Parameters: FP-SPLIT=FOUR, COMB=FOUR, STEP-PATT=7, DOPPLER=ON Number_of_Iterations: 1 Time_Per_Exposure: 1088.0S !(S/N=50 @ 17.8M) Special_Requirements: Comments: Lines = Fe II, Mn II !Line 16 Exposure_Number: 160 Target_Name: HD203664 Config: HRS Opmode: ACCUM Aperture: 2.0 Sp_Element: ECH-B Wavelength: 2851.9 Optional_Parameters: FP-SPLIT=FOUR, COMB=FOUR, STEP-PATT=7, DOPPLER=ON Number_of_Iterations: 1 Time_Per_Exposure: 979.2S !(S/N=50 @ 14.4M) Special_Requirements: Comments: Lines = Mg I !Line 17 Exposure_Number: 170 Target_Name: HD203664 Config: HRS Opmode: ACCUM Aperture: 2.0 Sp_Element: ECH-B Wavelength: 2800.0 Optional_Parameters: FP-SPLIT=FOUR, COMB=FOUR, STEP-PATT=7, DOPPLER=ON Number_of_Iterations: 1 Time_Per_Exposure: 761.6S !(S/N=50 @ 11.0M) Special_Requirements: Comments: Lines = Mg II !Line 18 Exposure_Number: 180 Target_Name: HD203664 Config: HRS Opmode: ACCUM Aperture: 2.0 Sp_Element: ECH-B Wavelength: 2260.8 Optional_Parameters: FP-SPLIT=FOUR, COMB=FOUR, STEP-PATT=7, DOPPLER=ON Number_of_Iterations: 1 ! Time_Per_Exposure: 979.2S !(S/N=50 @ 11.8M) Time_Per_Exposure: 1305.6S !(S/N=50 @ 11.8M) Special_Requirements: Comments: Lines = Fe II !Line 19 Exposure_Number: 190 Target_Name: HD203664 Config: HRS Opmode: ACCUM Aperture: 2.0 Sp_Element: ECH-B Wavelength: 2026.2 Optional_Parameters: FP-SPLIT=FOUR, COMB=FOUR, STEP-PATT=7, DOPPLER=ON Number_of_Iterations: 1 Time_Per_Exposure: 1414.4S !(S/N=50 @ 23.7M) Special_Requirements: Comments: Lines = Zn II, Mg I !Line 20 Exposure_Number: 200 Target_Name: HD203664 Config: HRS Opmode: ACCUM Aperture: 2.0 Sp_Element: G160M Wavelength: 1856.5 Optional_Parameters: FP-SPLIT=FOUR, COMB=FOUR, STEP-PATT=5, DOPPLER=ON Number_of_Iterations: 1 ! Time_Per_Exposure: 870.4S !(S/N=50 @ 14.8M) Time_Per_Exposure: 979.2SS !(S/N=50 @ 14.8M) Special_Requirements: Comments: Lines = Al III !Line 21 Exposure_Number: 210 Target_Name: HD203664 Config: HRS Opmode: ACCUM Aperture: 2.0 Sp_Element: G160M Wavelength: 1670.8 Optional_Parameters: FP-SPLIT=FOUR, COMB=FOUR, STEP-PATT=5, DOPPLER=ON Number_of_Iterations: 1 ! Time_Per_Exposure: 544.0S !(S/N=50 @ 8.3M) Time_Per_Exposure: 652.8S !(S/N=50 @ 8.3M) Special_Requirements: Comments: Lines = Al II Data_Distribution Medium: 8MM Blocking_Factor: 10 Ship_To: Kenneth Sembach Center for Space Research MIT 6-216 77 Massachusetts Avenue Cambridge, MA 02139 Ship_Via: UPS Recipient_Email: sembach@sundoggie.mit.edu