Recent Mass Ejection from Planetary-Nebula - Repeat for HOPR#55

Astronomy and Astrophysics – Astrophysics

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Hst Proposal Id #4778 Stellar Astrophysics

Scientific paper

This proposal is for repeat observations for the Cycle 1 program 2570. FOS observations were made incorrectly for this program, as described in HOPR no. 55, and we were authorized to submit up to 4.33 spacecraft hours of replacement time. We were moreover authorized to change the FOS time to imaging time for additional investigation of 0950+139, which is the central star of the planetary nebula EGB 6. We will use the WF/PC with V and I filters, in order to determine the colors of the close (0".18) companion discovered with the FOC images already obtained in this program. In addition, we will obtain WF/PC grism images in order to determine whether, as we suspect, this faint companion of the central star is an emission-line source.

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