High Angular Resolution Mid-IR Astronomy at Concordia

If we concentrate our attention on the study and the evolution of star forming processes rather than on the large scale structure, from the recent use of Large Telescopes in this context there are many examples of great interest. These include the study of the early phases of aggregation of matter (...

Full description

Bibliographic Details
Published in:Highlights of Astronomy
Main Author: Ferrari-Toniolo, Marco
Format: Article in Journal/Newspaper
Language:English
Published: Cambridge University Press (CUP) 2005
Subjects:
Online Access:http://dx.doi.org/10.1017/s1539299600017809
https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S1539299600017809
id crcambridgeupr:10.1017/s1539299600017809
record_format openpolar
spelling crcambridgeupr:10.1017/s1539299600017809 2023-05-15T14:05:47+02:00 High Angular Resolution Mid-IR Astronomy at Concordia Ferrari-Toniolo, Marco 2005 http://dx.doi.org/10.1017/s1539299600017809 https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S1539299600017809 en eng Cambridge University Press (CUP) https://www.cambridge.org/core/terms Highlights of Astronomy volume 13, page 964-964 ISSN 1539-2996 General Medicine journal-article 2005 crcambridgeupr https://doi.org/10.1017/s1539299600017809 2022-04-07T09:00:12Z If we concentrate our attention on the study and the evolution of star forming processes rather than on the large scale structure, from the recent use of Large Telescopes in this context there are many examples of great interest. These include the study of the early phases of aggregation of matter (stellar and planet formation), and the late phases of disaggregation during stellar evolution. In Fig 1, a spectacular example is shown of a high resolution image of an edge-on circumstellar disk of a young star (HR4796A), with respect to previous less resolved information (C.Telesco et al, Proc SPIE 4834, 101, 2002). A recent hypothesis of a Large Infrared Telescope called GTA (Grande Telescopio Antartico) has been proposed to the PNRA (Italian Plan for Antarctic Researches). This will require the following characteristics: high angular resolution in the mid-IR domain (large aperture); very high sensitivity (mainly due to the cold, dry conditions of the site); extreme simplicity in design and operational modes. The telescope will be a survey instrument and will be used almost without human intervention. The project examines the construction of a third tower at Dome C with the telescope configured to work in quasi-drift-scan without moving the enclosure and with a limited tracking time. In Fig 1, a sketch of the tower hosting the telescope is shown (M.F-T. et al, Proc SPIE 4836, 165, 2002). A study will be developed to determine the optimum configurations for observing in different bands, from the optical to the sub-mm range, with a refurbishment of the telescope and instrumentation during the summer break. Article in Journal/Newspaper Antarc* Antarctic antartic* Cambridge University Press (via Crossref) Antarctic Highlights of Astronomy 13 964 964
institution Open Polar
collection Cambridge University Press (via Crossref)
op_collection_id crcambridgeupr
language English
topic General Medicine
spellingShingle General Medicine
Ferrari-Toniolo, Marco
High Angular Resolution Mid-IR Astronomy at Concordia
topic_facet General Medicine
description If we concentrate our attention on the study and the evolution of star forming processes rather than on the large scale structure, from the recent use of Large Telescopes in this context there are many examples of great interest. These include the study of the early phases of aggregation of matter (stellar and planet formation), and the late phases of disaggregation during stellar evolution. In Fig 1, a spectacular example is shown of a high resolution image of an edge-on circumstellar disk of a young star (HR4796A), with respect to previous less resolved information (C.Telesco et al, Proc SPIE 4834, 101, 2002). A recent hypothesis of a Large Infrared Telescope called GTA (Grande Telescopio Antartico) has been proposed to the PNRA (Italian Plan for Antarctic Researches). This will require the following characteristics: high angular resolution in the mid-IR domain (large aperture); very high sensitivity (mainly due to the cold, dry conditions of the site); extreme simplicity in design and operational modes. The telescope will be a survey instrument and will be used almost without human intervention. The project examines the construction of a third tower at Dome C with the telescope configured to work in quasi-drift-scan without moving the enclosure and with a limited tracking time. In Fig 1, a sketch of the tower hosting the telescope is shown (M.F-T. et al, Proc SPIE 4836, 165, 2002). A study will be developed to determine the optimum configurations for observing in different bands, from the optical to the sub-mm range, with a refurbishment of the telescope and instrumentation during the summer break.
format Article in Journal/Newspaper
author Ferrari-Toniolo, Marco
author_facet Ferrari-Toniolo, Marco
author_sort Ferrari-Toniolo, Marco
title High Angular Resolution Mid-IR Astronomy at Concordia
title_short High Angular Resolution Mid-IR Astronomy at Concordia
title_full High Angular Resolution Mid-IR Astronomy at Concordia
title_fullStr High Angular Resolution Mid-IR Astronomy at Concordia
title_full_unstemmed High Angular Resolution Mid-IR Astronomy at Concordia
title_sort high angular resolution mid-ir astronomy at concordia
publisher Cambridge University Press (CUP)
publishDate 2005
url http://dx.doi.org/10.1017/s1539299600017809
https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S1539299600017809
geographic Antarctic
geographic_facet Antarctic
genre Antarc*
Antarctic
antartic*
genre_facet Antarc*
Antarctic
antartic*
op_source Highlights of Astronomy
volume 13, page 964-964
ISSN 1539-2996
op_rights https://www.cambridge.org/core/terms
op_doi https://doi.org/10.1017/s1539299600017809
container_title Highlights of Astronomy
container_volume 13
container_start_page 964
op_container_end_page 964
_version_ 1766277633012662272