Data

Abundance Analysis of New CEMP RR Lyrae Stars

The Australian National University
Kennedy, CR
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ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Adc&rfr_id=info%3Asid%2FANDS&rft_id=https://datacommons.anu.edu.au/DataCommons/item/anudc:5032&rft.title=Abundance Analysis of New CEMP RR Lyrae Stars&rft.identifier=https://datacommons.anu.edu.au/DataCommons/item/anudc:5032&rft.publisher=The Australian National University Data Commons&rft.description=Tonight, in the halo of the Galaxy, we observe variable carbon-enhanced metal-poor stars. These stars preserve chemical signatures of past stellar nucleosynthesis. We will use the WiFeS instrument in order to estimate accurate abundances of several elements. By doing so, we will determine how the first generations of stars produced the elements that surround us.&rft.creator=Kennedy, CR &rft.date=2013&rft_rights=All data obtained on ANU telescopes is publicly available after 12 months. Please contact the PI to negotiate access before that time.&rft_subject=ASTRONOMICAL AND SPACE SCIENCES&rft_subject=PHYSICAL SCIENCES&rft.type=dataset&rft.language=English Access the data
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All data obtained on ANU telescopes is publicly available after 12 months. Please contact the PI to negotiate access before that time.

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[email protected]

Full description

Tonight, in the halo of the Galaxy, we observe variable carbon-enhanced metal-poor stars. These stars preserve chemical signatures of past stellar nucleosynthesis. We will use the WiFeS instrument in order to estimate accurate abundances of several elements. By doing so, we will determine how the first generations of stars produced the elements that surround us.

Created: 2013-03-23

Data time period: 20 03 2013 to 22 03 2013

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Astronomical and Space Sciences | Physical Sciences |

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Identifiers
ACN 633 798 857