ISSN:
1572-9672
Keywords:
ISM: general
;
abundances
;
clouds
;
density
;
solar neighborhood
Source:
Springer Online Journal Archives 1860-2000
Topics:
Physics
Notes:
Abstract The distribution, kinematics and physical properties of the interstellar matter surrounding the Sun can be inferred from ground-based and UV spectroscopic observations. On a 200 pc scale the local interstellar matter appears inhomogeneous and asymmetric. Although it generally flows towards the lower density region, it is composed of numerous small components a few parsecs in size with slightly different velocities. On a smaller scale the extent and the nature of the Local Cloud which flows over the Sun are discussed based on HST-GHRS observations of nearby stars.
Type of Medium:
Electronic Resource
URL:
http://dx.doi.org/10.1007/BF00170810
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