Mid-infrared photometry of carbon stars and perspectives for surveys in the Magellanic Clouds from Dome-C

A preliminary analysis of the data from the MSX space infrared satellite, seems to confirm that the [8.8]-[12.5] micron color index is well correlated with the mass-loss rates in carbon stars of our Galaxy. The extension of this mid-infrared observation criterion to the Magellanic Clouds, with a sma...

Full description

Bibliographic Details
Main Authors: Ciprini, S, Busso, M
Language:English
Published: 2003
Subjects:
Astrophysics and Astronomy
Antarctic
The Antarctic
Antarc*
Online Access:http://cds.cern.ch/record/639124
id ftcern:oai:cds.cern.ch:639124
record_format openpolar
spelling ftcern:oai:cds.cern.ch:639124 2023-05-15T13:56:27+02:00 Mid-infrared photometry of carbon stars and perspectives for surveys in the Magellanic Clouds from Dome-C Ciprini, S Busso, M 2003-08-21 http://cds.cern.ch/record/639124 eng eng http://cds.cern.ch/record/639124 astro-ph/0308378 oai:cds.cern.ch:639124 Astrophysics and Astronomy 2003 ftcern 2018-07-28T06:06:11Z A preliminary analysis of the data from the MSX space infrared satellite, seems to confirm that the [8.8]-[12.5] micron color index is well correlated with the mass-loss rates in carbon stars of our Galaxy. The extension of this mid-infrared observation criterion to the Magellanic Clouds, with a small-size telescope, able to perform a continuous survey from Dome-C on the Antarctic Plateau, could be crucial to trace the local AGB population and evolution. Other/Unknown Material Antarc* Antarctic CERN Document Server (CDS) Antarctic The Antarctic
institution Open Polar
collection CERN Document Server (CDS)
op_collection_id ftcern
language English
topic Astrophysics and Astronomy
spellingShingle Astrophysics and Astronomy
Ciprini, S
Busso, M
Mid-infrared photometry of carbon stars and perspectives for surveys in the Magellanic Clouds from Dome-C
topic_facet Astrophysics and Astronomy
description A preliminary analysis of the data from the MSX space infrared satellite, seems to confirm that the [8.8]-[12.5] micron color index is well correlated with the mass-loss rates in carbon stars of our Galaxy. The extension of this mid-infrared observation criterion to the Magellanic Clouds, with a small-size telescope, able to perform a continuous survey from Dome-C on the Antarctic Plateau, could be crucial to trace the local AGB population and evolution.
author Ciprini, S
Busso, M
author_facet Ciprini, S
Busso, M
author_sort Ciprini, S
title Mid-infrared photometry of carbon stars and perspectives for surveys in the Magellanic Clouds from Dome-C
title_short Mid-infrared photometry of carbon stars and perspectives for surveys in the Magellanic Clouds from Dome-C
title_full Mid-infrared photometry of carbon stars and perspectives for surveys in the Magellanic Clouds from Dome-C
title_fullStr Mid-infrared photometry of carbon stars and perspectives for surveys in the Magellanic Clouds from Dome-C
title_full_unstemmed Mid-infrared photometry of carbon stars and perspectives for surveys in the Magellanic Clouds from Dome-C
title_sort mid-infrared photometry of carbon stars and perspectives for surveys in the magellanic clouds from dome-c
publishDate 2003
url http://cds.cern.ch/record/639124
geographic Antarctic
The Antarctic
geographic_facet Antarctic
The Antarctic
genre Antarc*
Antarctic
genre_facet Antarc*
Antarctic
op_relation http://cds.cern.ch/record/639124
astro-ph/0308378
oai:cds.cern.ch:639124
_version_ 1766263964824502272

Similar Items