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GRADES: A New Instrument for Spectroscopy of the Local Hot Gas

Published online by Cambridge University Press:  12 April 2016

M. Hurwitz ,
C. McKee ,
J. Edelstein ,
J. Vallerga ,
P. Jelinsky ,
M. Freyberg  and
D. Breitschwerdt
M. Hurwitz
Affiliation:
Space Sciences Laboratory, University of California, Berkeley, California 94720-7450, U.S.A.
C. McKee
Affiliation:
Space Sciences Laboratory, University of California, Berkeley, California 94720-7450, U.S.A.
J. Edelstein
Affiliation:
Space Sciences Laboratory, University of California, Berkeley, California 94720-7450, U.S.A.
J. Vallerga
Affiliation:
Space Sciences Laboratory, University of California, Berkeley, California 94720-7450, U.S.A.
P. Jelinsky
Affiliation:
Space Sciences Laboratory, University of California, Berkeley, California 94720-7450, U.S.A.
M. Freyberg
Affiliation:
Max-Planck-Institut für extraterrestrische Physik, D-85740 Garching, Germany
D. Breitschwerdt
Affiliation:
Max-Planck-Institut für extraterrestrische Physik, D-85740 Garching, Germany

Abstract

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Competing models for the origin of the local component of the diffuse X-ray background span more than an order of magnitude in temperature. We propose to test these models with a new instrument, the GRating Array Diffuse EUV Spectrometer (GRADES), which is sensitive to diffuse emission in the 90 – 260 Å bandpass, and offers a peak spectral resolution of about λ/127.

Type
Part III Observations and Modeling of the Local Bubble and the SXRB
Information
International Astronomical Union Colloquium , Volume 166: The Local Bubble and Beyond , 1997 , pp. 91 - 94
Copyright
Copyright © Springer-Verlag 1998

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