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Stellar and Galactic studies with the 2-m Himalayan Chandra Telescope

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dc.contributor.author Goswami, A
dc.date.accessioned 2020-11-26T15:43:11Z
dc.date.available 2020-11-26T15:43:11Z
dc.date.issued 2019-10
dc.identifier.citation Bulletin de la Societe Royale des Sciences de Liege, Vol. 88, pp. 198-206 en_US
dc.identifier.issn 0037-9565
dc.identifier.uri http://prints.iiap.res.in/handle/2248/7414
dc.description Open Access © Societe Royale des Sciences de Liege https://doi.org/10.25518/0037-9565.8843 en_US
dc.description.abstract The Himalayan Chandra Telescope (HCT), of the Indian Astronomical Observatory (IAO), is currently one of the most heavily subscribed telescopes in India. The telescope has been in regular use for scientific observations by national as well as international astronomical communities since May 2003. Over the past fifteen years, various observational programs have been carried out using HCT contributing to our understanding of many different aspects of stellar and Galactic astronomy. Here, a glimpse of spectroscopic studies made using HCT is provided with an aim to expand potential collaboration in the area of stellar and Galactic studies using these observing facilities. Some results from our long-term observing program on a search for CH stars from low resolution spectroscopy of high Galactic latitude objects that has given us the potential to discover objects of rare types are discussed. en_US
dc.language.iso en en_US
dc.publisher Societe Royale des Sciences de Liege en_US
dc.subject stars: carbon en_US
dc.subject stars: classification en_US
dc.subject stars: s-process elements en_US
dc.title Stellar and Galactic studies with the 2-m Himalayan Chandra Telescope en_US
dc.type Article en_US


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