The Diverse Properties of Type Icn Supernovae Point to Multiple Progenitor Channels

Autor: Pellegrino, C., Howell, D. A., Terreran, G., Arcavi, I., Bostroem, K. A., Brown, P. J., Burke, J., Dong, Y., Gilkis, A., Hiramatsu, D., Hosseinzadeh, G., McCully, C., Modjaz, M., Newsome, M., Gonzalez, E. Padilla, Pritchard, T. A., Sand, D. J., Valenti, S., Williamson, M.

Publikováno v: The Astrophysical Journal, Volume 938, page 73, 2020

We present a sample of Type Icn supernovae (SNe Icn), a newly-discovered class of transients characterized by their interaction with H- and He-poor circumstellar material (CSM). This sample is the largest collection of SNe Icn to date and includes ob

Externí odkaz: http://arxiv.org/abs/2205.07894

NWChem: Past, Present, and Future

Autor: Aprà, E., Bylaska, E. J., de Jong, W. A., Govind, N., Kowalski, K., Straatsma, T. P., Valiev, M., van Dam, H. J. J., Alexeev, Y., Anchell, J., Anisimov, V., Aquino, F. W., Atta-Fynn, R., Autschbach, J., Bauman, N. P., Becca, J. C., Bernholdt, D. E., Bhaskaran-Nair, K., Bogatko, S., Borowski, P., Boschen, J., Brabec, J., Bruner, A., Cauët, E., Chen, Y., Chuev, G. N., Cramer, C. J., Daily, J., Deegan, M. J. O., Dunning Jr., T. H., Dupuis, M., Dyall, K. G., Fann, G. I., Fischer, S. A., Fonari, A., Früuchtl, H., Gagliardi, L., Garza, J., Gawande, N., Ghosh, S., Glaesemann, K., Götz, A. W., Hammond, J., Helms, V., Hermes, E. D., Hirao, K., Hirata, S., Jacquelin, M., Jensen, L., Johnson, B. G., Jónsson, H., Kendall, R. A., Klemm, M., Kobayashi, R., Konkov, V., Krishnamoorthy, S., Krishnan, M., Lin, Z., Lins, R. D., Littlefield, R. J., Logsdail, A. J., Lopata, K., Ma, W., Marenich, A. V., del Campo, J. Martin, Mejia-Rodriguez, D., Moore, J. E., Mullin, J. M., Nakajima, T., Nascimento, D. R., Nichols, J. A., Nichols, P. J., Nieplocha, J., de la Roza, A. Otero, Palmer, B., Panyala, A., Pirojsirikul, T., Peng, B., Peverati, R., Pittner, J., Pollack, L., Richard, R. M., Sadayappan, P., Schatz, G. C., Shelton, W. A., Silverstein, D. W., Smith, D. M. A., Soares, T. A., Song, D., Swart, M., Taylor, H. L., Thomas, G. S., Tipparaju, V., Truhlar, D. G., Tsemekhman, K., Van Voorhis, T., Vázquez-Mayagoitia, Á., Verma, P., Villa, O., Vishnu, A., Vogiatzis, K. D., Wang, D., Weare, J. H., Williamson, M. J., Windus, T. L., Woliński, K., Wong, A. T., Wu, Q., Yang, C., Yu, Q., Zacharias, M., Zhang, Z., Zhao, Y., Harrison, R. J.

Publikováno v: J. Chem. Phys., 152, 184102 (2020)

Specialized computational chemistry packages have permanently reshaped the landscape of chemical and materials science by providing tools to support and guide experimental efforts and for the prediction of atomistic and electronic properties. In this

Externí odkaz: http://arxiv.org/abs/2004.12023

The Feasibility of Deriving the Electronic Frailty Index from Australian General Practice Records

Autor: Lewis ET, Williamson M, Lewis LP, Ní Chróinín D, Dent E, Ticehurst M, Peters R, Macniven R, Cardona M

Publikováno v: Clinical Interventions in Aging, Vol Volume 17, Pp 1589-1598 (2022)

Ebony T Lewis,1– 3 Margaret Williamson,1,4 Lou P Lewis,5 Danielle Ní Chróinín,6,7 Elsa Dent,8 Maree Ticehurst,5,9 Ruth Peters,2,3 Rona Macniven,1 Magnolia Cardona10,11 1School of Population Health, Faculty of Medicine & Health, University of New

Externí odkaz: https://doaj.org/article/0f0dcfd58f4a4c88aa5d15620fad9af3

Kepler sheds new and unprecedented light on the variability of a blue supergiant: gravity waves in the O9.5Iab star HD 188209

Autor: Aerts, C., Simon-Diaz, S., Bloemen, S., Debosscher, J., Papics, P. I., Bryson, S., Still, M., Moravveji, E., Williamson, M. H., Grundahl, F., Andersen, M. Fredslund, Antoci, V., Palle, P. L., Christensen-Dalsgaard, J., Rogers, T. M.

Publikováno v: A&A 602, A32 (2017)

Stellar evolution models are most uncertain for evolved massive stars. Asteroseismology based on high-precision uninterrupted space photometry has become a new way to test the outcome of stellar evolution theory and was recently applied to a multitud

Externí odkaz: http://arxiv.org/abs/1703.01514

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