Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-25T22:52:12.992Z Has data issue: false hasContentIssue false

AMBER/VLTI Snapshot Survey on Circumstellar Environments

Published online by Cambridge University Press:  23 January 2015

Th. Rivinius
Affiliation:
ESO - European Organisation for Astronomical Research in the Southern Hemisphere, Chile email: [email protected]
W.J. de Wit
Affiliation:
ESO - European Organisation for Astronomical Research in the Southern Hemisphere, Chile email: [email protected]
Z. Demers
Affiliation:
Department of Physics and Astronomy, The University of Western Ontario, London, Canada Landessternwarte Königstuhl, D-69117, Heidelberg, Germany
A. Quirrenbach
Affiliation:
Landessternwarte Königstuhl, D-69117, Heidelberg, Germany
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

OHANA is an interferometric snapshot survey of the gaseous circumstellar environments of hot stars, carried out by the VLTI group at the Paranal observatory. It aims to characterize the mass-loss dynamics (winds/disks) at unexplored spatial scales for many stars. The survey employs the unique combination of AMBER's high spectral resolution with the unmatched spatial resolution provided by the VLTI. Because of the spatially unresolved central OBA-type star, with roughly neutral colour terms, their gaseous environments are among the easiest objects to be observed with AMBER, yet the extent and kinematics of the line emission regions are of high astrophysical interest.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2015 

References

Chelli, A., Utrera, O. H., & Duvert, G. 2009, A&A 502, 705Google Scholar
Petrov, R. G., Malbet, F., Weigelt, G., et al. 2007, A&A 464, 1Google Scholar
Tatulli, E., Millour, F., Chelli, A., et al. 2007, A&A 464, 29Google Scholar