Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Schlaufman, KC"'
Autor:
Casey, AR, Ho, AYQ, Ness, M, Hogg, DW, Rix, HW, Angelou, GC, Hekker, S, Tout, CA, Lattanzio, JC, Karakas, AI, Woods, TE, Price-Whelan, AM, Schlaufman, KC
Theoretical models of stellar evolution predict that most of the lithium inside a star is destroyed as the star becomes a red giant. However, observations reveal that about 1% of red giants are peculiarly rich in lithium, often exceeding the amount i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2b7b34b15187afc679e16f4d3da8648c
Autor:
Kemp, AJ, Casey, AR, Miles, MT, Norfolk, BJ, Lattanzio, JC, Karakas, AI, Schlaufman, KC, Ho, AYQ, Tout, CA, Ness, M, Ji, AP
Stars with unusual elemental abundances offer clues about rare astrophysical events or nucleosynthetic pathways. Stars with significantly depleted magnesium and enhanced potassium ([Mg/Fe] < -0.5; [K/Fe] > 1) have to date only been found in the massi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::90c23029e2576a829b0ab8b91f61c342
Autor:
Saskia Hekker, Christopher A. Tout, Adrian M. Price-Whelan, Tyrone E. Woods, John C. Lattanzio, Hans-Walter Rix, Amanda I. Karakas, Melissa Ness, George C. Angelou, Kevin C. Schlaufman, Andrew R. Casey, David W. Hogg, Anna Y. Q. Ho
Publikováno v:
The Astrophysical Journal
Casey, A R, Ho, A Y Q, Ness, M, Hogg, D W, Rix, H-W, Angelou, G C, Hekker, S, Tout, C A, Lattanzio, J C, Karakas, A, Woods, T E, Price-Whelan, A M & Schlaufman, K C 2019, ' Tidal Interactions between Binary Stars Can Drive Lithium Production in Low-mass Red Giants ', Astrophysical Journal, vol. 880, no. 2, 125 . https://doi.org/10.3847/1538-4357/ab27bf
Casey, A R, Ho, A Y Q, Ness, M, Hogg, D W, Rix, H-W, Angelou, G C, Hekker, S, Tout, C A, Lattanzio, J C, Karakas, A, Woods, T E, Price-Whelan, A M & Schlaufman, K C 2019, ' Tidal Interactions between Binary Stars Can Drive Lithium Production in Low-mass Red Giants ', Astrophysical Journal, vol. 880, no. 2, 125 . https://doi.org/10.3847/1538-4357/ab27bf
Theoretical models of stellar evolution predict that most of the lithium inside a star is destroyed as the star becomes a red giant. However, observations reveal that about 1% of red giants are peculiarly rich in lithium, often exceeding the amount i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::40e9e177b2b10b4be64350cebd1c48d2
http://arxiv.org/abs/1902.04102
http://arxiv.org/abs/1902.04102