File Download

There are no files associated with this item.

  Links for fulltext
     (May Require Subscription)
  • Find via Find It@HKUL
Supplementary

Conference Paper: Zooming into the complex dusty envelopes of C-rich AGB stars

TitleZooming into the complex dusty envelopes of C-rich AGB stars
Authors
Issue Date2019
PublisherCambridge University Press. The Journal's web site is located at http://journals.cambridge.org/action/displayJournal?jid=IAU
Citation
IAU Symposium 343: Why Galaxies Care About AGB Stars: A Continuing Challenge through Cosmic Time, Vienna, Austria, 20- 23 August 2018. In Proceedings of the International Astronomical Union How to Cite?
AbstractRecent advances in high-angular resolution instruments (VLT and VLTI, ALMA) have enabled us to delve deep into the circumstellar envelopes of AGB stars from the optical to the sub-mm wavelengths, thus allowing us to study in detail the gas and dust formation zones (e.g., their geometry, chemistry and kinematics). This project focuses on four (4) C-rich AGB stars observed with a high-angular resolution technique in the near-infrared: a multi-wavelength tomographic study of the dusty layers of the circumstellar envelopes of these C-rich stars, i.e. the variations in the morphology and temperature distribution.
DescriptionPoster presentation
Persistent Identifierhttp://hdl.handle.net/10722/260837
ISSN
2023 SCImago Journal Rankings: 0.121

 

DC FieldValueLanguage
dc.contributor.authorLykou, F-
dc.contributor.authorHron, J-
dc.contributor.authorKlotz, D-
dc.date.accessioned2018-09-14T08:48:17Z-
dc.date.available2018-09-14T08:48:17Z-
dc.date.issued2019-
dc.identifier.citationIAU Symposium 343: Why Galaxies Care About AGB Stars: A Continuing Challenge through Cosmic Time, Vienna, Austria, 20- 23 August 2018. In Proceedings of the International Astronomical Union-
dc.identifier.issn1743-9213-
dc.identifier.urihttp://hdl.handle.net/10722/260837-
dc.descriptionPoster presentation-
dc.description.abstractRecent advances in high-angular resolution instruments (VLT and VLTI, ALMA) have enabled us to delve deep into the circumstellar envelopes of AGB stars from the optical to the sub-mm wavelengths, thus allowing us to study in detail the gas and dust formation zones (e.g., their geometry, chemistry and kinematics). This project focuses on four (4) C-rich AGB stars observed with a high-angular resolution technique in the near-infrared: a multi-wavelength tomographic study of the dusty layers of the circumstellar envelopes of these C-rich stars, i.e. the variations in the morphology and temperature distribution.-
dc.languageeng-
dc.publisherCambridge University Press. The Journal's web site is located at http://journals.cambridge.org/action/displayJournal?jid=IAU-
dc.relation.ispartofProceedings of the International Astronomical Union-
dc.rightsProceedings of the International Astronomical Union. Copyright © Cambridge University Press.-
dc.rightsThis article has been published in a revised form in [Journal] [http://doi.org/XXX]. This version is free to view and download for private research and study only. Not for re-distribution, re-sale or use in derivative works. © copyright holder.-
dc.titleZooming into the complex dusty envelopes of C-rich AGB stars-
dc.typeConference_Paper-
dc.identifier.emailLykou, F: lykoufc@hku.hk-
dc.identifier.hkuros290539-
dc.publisher.placeUnited Kingdom-
dc.identifier.issnl1743-9213-

Export via OAI-PMH Interface in XML Formats


OR


Export to Other Non-XML Formats