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pro vyhledávání: '"Camacho, Yssavo"'
Autor:
Marion, G. H., Brown, Peter J., Vinkó, Jozsef, Silverman, Jeffrey M., Sand, David J., Challis, Peter, Kirshner, Robert P., Wheeler, J. Craig, Berlind, Perry, Brown, Warren R., Calkins, Michael L., Camacho, Yssavo, Dhungana, Govinda, Foley, Ryan J., Friedman, Andrew S., Graham, Melissa L., Howell, D. Andrew, Hsiao, Eric Y., Irwin, Jonathan M., Jha, Saurabh W., Kehoe, Robert, Macri, Lucas M., Maeda, Keiichi, Mandel, Kaisey, McCully, Curtis, Pandya, Viraj, Rines, Kenneth J., Wilhelmy, Steven, Zheng, Weikang
We report evidence for excess blue light from the Type Ia supernova SN 2012cg at fifteen and sixteen days before maximum B-band brightness. The emission is consistent with predictions for the impact of the supernova on a non-degenerate binary compani
Externí odkaz:
http://arxiv.org/abs/1507.07261
Autor:
Childress, Michael J., Hillier, D. John, Seitenzahl, Ivo, Sullivan, Mark, Maguire, Kate, Taubenberger, Stefan, Scalzo, Richard, Ruiter, Ashley, Blagorodnova, Nadejda, Camacho, Yssavo, Castillo, Jayden, Elias-Rosa, Nancy, Fraser, Morgan, Gal-Yam, Avishay, Graham, Melissa, Howell, D. Andrew, Inserra, Cosimo, Jha, Saurabh W., Kumar, Sahana, Mazzali, Paolo A., McCully, Curtis, Morales-Garoffolo, Antonia, Pandya, Viraj, Polshaw, Joe, Schmidt, Brian, Smartt, Stephen, Smith, Ken W., Sollerman, Jesper, Spyromilio, Jason, Tucker, Brad, Valenti, Stefano, Walton, Nicholas, Wolf, Christian, Yaron, Ofer, Young, D. R., Yuan, Fang, Zhang, Bonnie
The light curves of Type Ia supernovae (SNe Ia) are powered by the radioactive decay of $^{56}$Ni to $^{56}$Co at early times, and the decay of $^{56}$Co to $^{56}$Fe from ~60 days after explosion. We examine the evolution of the [Co III] 5892 A emis
Externí odkaz:
http://arxiv.org/abs/1507.02501
Akademický článek
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