An EUV Observation of Capella

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

We have observed the star Capella with an EUV spectrograph from 200-340 Angstroms. The primary emission line in this wavelength region was anticipated to be HeII 304 Angstroms. However, no emission at any wavelength in the bandpass was detected. We will present the deduced limits on 304 Angstroms emission from Capella, and the implications regarding the interstellar medium towards Capella and regarding possible emission schemes in Capella.

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