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http://hdl.handle.net/2248/7707
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DC Field | Value | Language |
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dc.contributor.author | Bharat Kumar, Yerra | - |
dc.contributor.author | Reddy, B. E | - |
dc.date.accessioned | 2021-06-25T13:30:54Z | - |
dc.date.available | 2021-06-25T13:30:54Z | - |
dc.date.issued | 2020-12 | - |
dc.identifier.citation | Journal of Astrophysics and Astronomy, Vol. 41, No. 1, 49 | en_US |
dc.identifier.issn | 0973-7758 | - |
dc.identifier.uri | http://hdl.handle.net/2248/7707 | - |
dc.description | Restricted Access | en_US |
dc.description | The original publication is available at springerlink.com | - |
dc.description.abstract | The overabundance of lithium in low-mass red giants has been a topic of interest for over four decades. Low-mass stars are expected to destroy lithium gradually throughout their lifetimes. Against this expectation, about 1% of red giants in the Galaxy show anomalously large Li which, in the literature, areknown as lithium-rich giants. The advent of large-scale stellar surveys (LAMOST, GALAH, Kepler, Gaia) coupled with high-resolution spectra enabled to find important clues about Li enhancement origin in redgiants. These new studies suggest Li enhancement is mostly associated with the red clump region, post-Heflash. Here, we will describe our recent results along with current updates in the field. | en_US |
dc.language.iso | en | en_US |
dc.publisher | Indian Academy of Sciences | en_US |
dc.relation.uri | https://doi.org/10.1007/s12036-020-09660-9 | - |
dc.rights | © Indian Academy of Sciences | - |
dc.subject | Late-type stars | en_US |
dc.subject | Stellar evolution | en_US |
dc.subject | Abundances-lithium | en_US |
dc.title | Evolution of lithium in low-mass giants: an observational perspective | en_US |
dc.type | Article | en_US |
Appears in Collections: | IIAP Publications |
Files in This Item:
File | Description | Size | Format | |
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Evolution of lithium in low-mass giants an observational perspective.pdf Restricted Access | 593.91 kB | Adobe PDF | View/Open Request a copy |
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