Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001mnras.327..841c&link_type=abstract
Monthly Notices of the Royal Astronomical Society, Volume 327, Issue 3, pp. 841-848.
Astronomy and Astrophysics
Astronomy
15
Line: Profiles, Stars: Individual: Alpha Oph, Ism: Structure
Scientific paper
I present very high resolution (R=400000 and R=880000) observations of interstellar Caii absorption lines towards eight early-type stars situated within 15° of α Oph on the sky. I confirm an earlier result that the interstellar structure responsible for the anomalously strong Caii absorption towards α Oph has a spatial extent of <~1pc (and is probably very much smaller). Many discrete interstellar absorption components are apparent in these high-resolution data, but while several have velocities in the range expected for the local interstellar medium (LISM), no convincing detections of either the local interstellar cloud (LIC), or the so-called G cloud, were made. In the former case, I argue that the relatively weak LIC components are masked by components arising in more distant clouds, but which have LISM-like velocities owing to the pervasive influence of outflow from the Sco-Cen association. The non-detection of the G cloud is more problematical, and I tentatively argue that, previous claims notwithstanding, this feature does not extend to galactic latitudes as high as +15° in this direction.
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