HST STIS Spectra of the Central Stars of Three Orion Proplyds

Details HST STIS Spectra of the Central Stars of Three Orion Proplyds HST STIS Spectra of the Central Stars of Three Orion Proplyds

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...20510512m&link_type=abstract

American Astronomical Society Meeting 205, #105.12; Bulletin of the American Astronomical Society, Vol. 36, p.1519

Astronomy and Astrophysics

Astronomy

Scientific paper

We have obtained the first spectra of central stars of proplyds. Spectra were obtained using the Hubble Space Telescope STIS with the 52 arcsec x 0.5 arcsec slit and G750L grating, giving a resolution of 790, centered at 7751A with a bandpass from 5236A to 10266A. We describe the spectrum extraction method and present the extracted spectra and spectral types for the central stars of 164-510, 171-340, and 218-354. Using their spectral classifications, we compare them with theoretical pre-MS evolutionary models.

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