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Communication Dans Un Congrès Année : 2011

A High Velocity Cloud Detected Towards M13

Résumé

We present HST-COS observations of the interstellar sight-line towards the M13 globular cluster. High velocity gas at V -120 km/s and intermediate velocity gas at V -65 km/s has been detected in many UV absorption lines. The HVC gas is probably associated with the Complex K IVC with a distance of 1.0 < z < 4.7 kpc. This would place the infalling HVC gas far closer than previous estimates of HV clouds surrounding our Galaxy.
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hal-03743907 , version 1 (02-08-2022)

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Barry Y. Welsh, Rosine Lallement, Jonathan Wheatley. A High Velocity Cloud Detected Towards M13. American Astronomical Society, AAS Meeting #217, Jan 2011, Seattle, WA, United States. ⟨hal-03743907⟩
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