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pro vyhledávání: '"Goldwasser, Samantha"'
Autor:
Sharma, Yashvi, Sollerman, Jesper, Fremling, Christoffer, Kulkarni, Shrinivas R., De, Kishalay, Irani, Ido, Schulze, Steve, Strotjohann, Nora Linn, Gal-Yam, Avishay, Maguire, Kate, Perley, Daniel A., Bellm, Eric C., Kool, Erik C., Brink, Thomas, Bruch, Rachel, Deckers, Maxime, Dekany, Richard, Dugas, Alison, Goldwasser, Samantha, Graham, Matthew J., Graham, Melissa L., Groom, Steven L., Hankins, Matt, Jencson, Jacob, Johansson, Joel P., Karambelkar, Viraj, Kasliwal, Mansi M., Masci, Frank J., Medford, Michael S., Neill, James D., Nir, Guy, Riddle, Reed L., Rigault, Mickael, Schweyer, Tassilo, Terwel, Jacco H., Yan, Lin, Yang, Yi, Yao, Yuhan
Among the supernovae (SNe) that show strong interaction with the circumstellar medium, there is a rare subclass of Type Ia supernovae, SNe Ia-CSM, that show strong narrow hydrogen emission lines much like SNe IIn but on top of a diluted over-luminous
Externí odkaz:
http://arxiv.org/abs/2301.04637
Autor:
Strotjohann, Nora L., Ofek, Eran O., Gal-Yam, Avishay, Bruch, Rachel, Schulze, Steve, Shaviv, Nir, Sollerman, Jesper, Filippenko, Alexei V., Yaron, Ofer, Fremling, Christoffer, Nordin, Jakob, Kool, Erik C., Perley, Dan A., Ho, Anna Y. Q., Yang, Yi, Yao, Yuhan, Soumagnac, Maayane T., Graham, Melissa L., Barbarino, Cristina, Tartaglia, Leonardo, De, Kishalay, Goldstein, Daniel A., Cook, David O., Brink, Thomas G., Taggart, Kirsty, Yan, Lin, Lunnan, Ragnhild, Kasliwal, Mansi, Kulkarni, Shri R., Nugent, Peter E., Masci, Frank J., Rosnet, Philippe, Adams, Scott M., Andreoni, Igor, Bagdasaryan, Ashot, Bellm, Eric C., Burdge, Kevin, Duev, Dmitry A., Dugas, Alison, Frederick, Sara, Goldwasser, Samantha, Hankins, Matthew, Irani, Ido, Karambelkar, Viraj, Kupfer, Thomas, Liang, Jingyi, Neill, James D., Porter, Michael, Riddle, Reed L., Sharma, Yashvi, Short, Phil, Taddia, Francesco, Tzanidakis, Anastasios, van Roestel, Jan, Walters, Richard, Zhuang, Zhuyun
Publikováno v:
ApJ 907 99 (2021)
Interaction-powered supernovae (SNe) explode within an optically-thick circumstellar medium (CSM) that could be ejected during eruptive events. To identify and characterize such pre-explosion outbursts we produce forced-photometry light curves for 19
Externí odkaz:
http://arxiv.org/abs/2010.11196
Akademický článek
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