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163“... analysis indicates that for stars with [Fe/H] ≤–2.0, 20% exhibit [C/Fe] ≥+0.7. This fraction increases...”
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164by LHCb Collaboration, Boettcher, Thomas Julian, Craik, D. C., Weisser, Constantin, Williams, MichaelGet full text
Published 2020
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169by Boettcher, Thomas Julian, Craik, Daniel C, Kitouni, Ouail, Weisser, Constantin, Williams, Michael“... to be necessary to include new spin-0 and spin-1 resonances in the D-K+ channel with masses around 2.9 GeV/c2...”
Published 2022
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170by Hansen, T., Hansen, C. J., Christlieb, N., Beers, T. C., Yong, D., Bessell, M. S., Placco, V. M., Norris, J. E., Asplund, M., Frebel, Anna L., Perez Garcia, A. E.“... that constrain the possible astrophysical sites of element production, including Li, C, N, O, the α-elements...”
Published 2015
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171by Fox, W., Igumenshchev, I., Town, R. P. J., Stoeckl, C., Glebov, V., Rosenberg, Michael Jonathan, Li, C. K., Seguin, Fredrick Hampton, Frenje, Johan A, Petrasso, Richard DGet full text
Published 2017
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172by Leibrandt, David Ray, Labaziewicz, Jaroslaw, Clark, Robert J., Chuang, Isaac L., Edpstein, R. J., Ospelkaus, C., Wesenberg, J. H., Bollinger, J. J., Leibfried, D., Wineland, D. J., Stick, D., Sterk, J., Monroe, C., Pai, C.-S., Low, Y., Frahm, R., Slusher, R. E.Get full text
Published 2014
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173by Tzeferacos, P., Lamb, D., Gregori, G., Norreys, P. A., Follett, R. K., Froula, D. H., Koenig, M., Amendt, P. A., Park, H. S., Remington, B. A., Ryutov, D. D., Wilks, S. C., Betti, R., Frank, A., Hu, S. X., Sangster, T. C., Hartigan, P., Drake, R. P., Kuranz, C. C., Lebedev, S. V., Woolsey, N. C., Li, Chikang, Rosenberg, Michael Jonathan, Frenje, Johan A, Rinderknecht, Hans George, Sio, Hong Weng, Zylstra, Alex Bennett, Petrasso, Richard D, Seguin, Fredrick HamptonGet full text
Published 2017
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174by Hansen, T., Hansen, C. J., Christlieb, N., Yong, D., Bessell, M. S., Beers, Timothy C., Placco, V. M., Norris, J. E., Asplund, M., Frebel, Anna L., Garcia Perez, A. E.“... in the sample, HE 0233–0343 ([Fe/H] = –4.68), is a subgiant with a carbon enhancement of [C/Fe] = +3.5, slightly...”
Published 2015
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175by Strohmayer, T. E., Arzoumanian, Z., Bogdanov, S., Bult, P. M., Enoto, T., Gendreau, K. C., Guillot, S., Harding, A. K., Ho, W. C. G., Homan, J., Jaisawal, G. K., Keek, L., Kerr, M., Mahmoodifar, S., Markwardt, C. B., Ransom, S. M., Ray, P. S., Wolff, M. T., Chakrabarty, Deepto, Remillard, Ronald AGet full text
Published 2019
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176by Amendt, P. A., Atzeni, S., Hoffman, N. M., Glebov, V. Yu., Stoeckl, C., Seka, W., Marshall, F. J., Delettrez, J. A., Sangster, T. C., Betti, R., Wilks, S. C., Pino, J., Kagan, G., Molvig, K., Nikroo, A., Rosenberg, Michael Jonathan, Seguin, Fredrick Hampton, Rinderknecht, Hans George, Zylstra, Alex Bennett, Li, C. K., Sio, Hong Weng, Gatu Johnson, Maria, Frenje, Johan A, Petrasso, Richard DGet full text
Published 2017
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