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The Thermal Pressure of the Interstellar Medium Derived from Cloud Shadows in the Extreme Ultraviolet

Published online by Cambridge University Press:  12 April 2016

Thomas W. Berghöfer
Affiliation:
Space Sciences Laboratory, University of California, Berkeley, CA 94720, USA
Stuart Bowyer
Affiliation:
Space Sciences Laboratory, University of California, Berkeley, CA 94720, USA
Richard Lieu
Affiliation:
Department of Physics, University of Alabama, Huntsville, USA
Jens Knude
Affiliation:
Niels Bohr Institute for Astronomy, Physics, and Geophysics, University Observatory, Juliane Mariesvej 30, DK-2100 Copenhagen OE, Denmark

Abstract

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We have used the Deep Survey telescope of EUVE to investigate shadows in the diffuse EUV/Soft X-ray background cast by clouds in the interstellar medium. We confirm the existence of a shadow previously reported, and provide evidence for two new shadows. We used IRAS data to identify the clouds producing these shadows and to determine their optical depth to EUV radiation. The EUV-absorbing clouds are optically thick in the EUV, and all EUV emission detected in the direction of these shadows must be produced from material in front of the clouds. We obtained new optical data to determine the distance to these clouds. We use a new differential cloud technique to obtain the pressure of the interstellar medium. These results do not depend on any zero level calibration of the data. Our results provide evidence that the pressure of the hot interstellar gas is the same in three different directions in the local interstellar medium, and is at least 8 times higher than derived for the local cloud surrounding our Sun. This provides new evidence for large thermal pressure imbalances in the local ISM, and directly contradicts the basic assumption of thermal pressure equilibrium used in almost all present models of the interstellar medium.

Type
Part II UV and Soft X-ray Observations of the LISM
Copyright
Copyright © Springer-Verlag 1998

References

Bowyer, S., Lieu, R., Sidher, S.D., Lampton, M., Knude, J. 1995, Nature, 375, 212 Google Scholar
Breitschwerdt, D., Schmutzler, T., 1994, Nature, 371, 774 Google Scholar
Frisch, P.C., 1995, Space Sci. Rev., 72, 499 CrossRefGoogle Scholar
McKee, C.F., Ostriker, J.P., 1977, ApJ, 218, 148 Google Scholar
Vallerga, J., 1996, Space Sci. Rev., 78, 277 Google Scholar