ORFEUS II echelle spectra: The scale height of interstellar O VI in the halo

FUV high resolution spectra of 18 stars, particularly chosen to observe the interstellar medium (ISM), were obtained during the second ORFEUS-SPAS free flight space shuttle mission in December 1996. Among these were 6 objects with a distance to the galactic plane larger than 1 kpc, one SMC and 4 LMC...

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Bibliographic Details
Published in:arXiv.org 1998-08
Main Authors: Widmann, H, de Boer, K S, Richter, P, Kraemer, G, Appenzeller, I, Barnstedt, J, Goelz, M, Grewing, M, Gringel, W, Mandel, H, Werner, K
Format: Article
Language:English
Subjects:
Free flight
Interstellar matter
Magellanic clouds
Probability distribution functions
Scale height
Space shuttle
Spas
Spectra
Stars
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Summary:FUV high resolution spectra of 18 stars, particularly chosen to observe the interstellar medium (ISM), were obtained during the second ORFEUS-SPAS free flight space shuttle mission in December 1996. Among these were 6 objects with a distance to the galactic plane larger than 1 kpc, one SMC and 4 LMC stars. This selction of targets is part of the ORFEUS program to explore the galactic halo. As the most important tracer of the hot gas we analyzed the stronger component of the important O VI doublet in all our ISM spectra. We found an average N(O VI) x sin |b| = 3.5 x 10^14 /cm^2 on the lines of sight to the 4 LMC stars. Assuming an exponential distribution of O VI we calculated a midplane density n(o) of 2.07 x 10^-8 /cm^3 and a scle height h(o) of 5.50 kpc. (Research supported in part by the DARA)
ISSN:2331-8422