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We used the FUSE (Far Ultraviolet Spectroscopic Explorer) satellite to observe OVI emission along two sightlines towards the edge of the interaction zone (IZ) between the Loop I superbubble and the Local Bubble. One sightline was chosen because mater
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7982647ac0ad35460d18ba97da4d625b
http://arxiv.org/abs/0805.2972
http://arxiv.org/abs/0805.2972
