! +====================+ ! | PED OUTPUT PRODUCT | ! +====================+ ! ! /spectre/data1/aroman/proposals/6492.prop ! Generated by PREPROCESSOR, version 6.3g ! Date: Mon Jul 29 14:19:53 EDT 1996 Proposal_Information Title: High Resolution Imaging of the Massive Overcontact Binary RY Scuti Proposal_Category: GO Scientific_Category: BINARIES AND STAR FORMATION Cycle: 6 Investigators PI_Name: Robert Gehrz PI_Institution: University of Minnesota CoI_Name: Terry Jones CoI_Institution: University of Minnesota Contact: Y CoI_Name: Roberta Humphreys CoI_Institution: University of Minnesota Contact: CoI_Name: Kris Davidson CoI_Institution: University of Minnesota Contact: CoI_Name: Joachim Krautter CoI_Institution: University of Heidelberg Contact: Abstract: RY Scuti is a post-main sequence, eclipsing, 'overcontact' binary. The two components are very massive, 49 and 39 M_\odot , with a combined luminosity in excess of 3* 10^6L_\odot . Ground based observations have established that this star is surrounded with a very unusual nebula about 1 arcsecond in extent containing both ionized gas and thermally emitting dust. The Ne abundance in the nebula is well above solar composition, indicating the system is at a critical phase of its evolution. We propose to image the nebulosity around RY Scuti to investigate its morphology and the mass loss process in the system. We will use these images to distinguish between hypothesized mass loss scenarios and to study the interface between the plasma and dust regions of the nebula. Questions Observing_Description: RY Scuti is a relatively bright object (V = 9.1, B = 10.1) surrounded by faint nebulosity. We have planned a series of exposures in V (F547M), B (F467M) and HAlpha (F656N) with the shortest chosen to avoid bleeding from the central star and the longest to image the fainter outer parts of the nebula. The exposure times are: 0.5s, 3s, 20s, 60s in V; 10s, 50s, 250s in B; 15s, 75s, 400s in HAlpha . With standard allowances for acquisition and overhead time this fills one orbit. begintabularlll Cycle 6 & Primary Orbits:1 & Exposures:10, endtabular Real_Time_Justification: None. R. D. Gehrz and J. Krautter will be obtaining supporting ground-based near-IR imaging observations using IRAC-2 on the 2.3-m telescope and mid-IR imaging observations using the TIMMI camera on the 3.6-m telescope at ESO. Calibration_Justification: Additional_Comments: Fixed_Targets Target_Number: 100 Target_Name: HD169515 Alternate_Names: RYScuti Description: STAR,SUPERGIANT O,INTERACTING BINARY Position: RA=18H 22M 42.706S +/- 0.0011S,DEC=-12D 43' 9.24" +/- 0.005" Equinox: 1950 RV_or_Z: RA_PM: Dec_PM: Epoch: Annual_Parallax: Flux: V = 9.1+/-0.1 B-V = 1.06+/-0.05 E(B-V) = 1.37+/-0.1 Comments: Solar_System_Targets Generic_Targets Scan_Data Visits Visit_Number: 01 Visit_Requirements: On_Hold_Comments: Visit_Comments: Exposure_Number: 101 Target_Name: HD169515 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F467M Wavelength: Optional_Parameters: ATD-GAIN=15 Number_of_Iterations: 1 Time_Per_Exposure: 2 S Special_Requirements: SEQ 101-303 NON-INT Comments: Exposure_Number: 102 Target_Name: HD169515 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F467M Wavelength: Optional_Parameters: DITHER-TYPE=LINE,DITHER-LINE-SPACING=0.161 Number_of_Iterations: 2 Time_Per_Exposure: 100 S Special_Requirements: Comments: Exposure_Number: 301 Target_Name: HD169515 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F656N Wavelength: Optional_Parameters: ATD-GAIN=15 Number_of_Iterations: 1 Time_Per_Exposure: 5 S Special_Requirements: Comments: Exposure_Number: 302 Target_Name: HD169515 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F656N Wavelength: Optional_Parameters: Number_of_Iterations: 2 Time_Per_Exposure: 20 S Special_Requirements: Comments: Exposure_Number: 303 Target_Name: HD169515 Config: WFPC2 Opmode: IMAGE Aperture: PC1 Sp_Element: F656N Wavelength: Optional_Parameters: DITHER-TYPE=LINE,DITHER-LINE-SPACING=0.161 Number_of_Iterations: 1 Time_Per_Exposure: 120 S Special_Requirements: Comments: Data_Distribution ! Defaults indicated; change if desired Medium: 8MM Blocking_Factor: 10 Ship_To: PI_Address Ship_Via: UPS Recipient_Email: ! Let us know what you think of this template and software! ! Please send a list of your likes and dislikes to your Program Coordinator