Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Nyholm, Anders"'
Autor:
Nyholm, Anders
Astronomi fascinerar många och har spelat en avgörande roll i fysikens utveckling. I det svenska gymnasiets läroplan Gy2011 ingår astronomi i kursen Fysik 2. Tidigare intervjustudier har visat att lärare som undervisar i Fysik 2 ofta ger astrono
Externí odkaz:
http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-194829
Autor:
Schulze, Steve, Yaron, Ofer, Sollerman, Jesper, Leloudas, Giorgos, Gal, Amit, Wright, Angus H., Lunnan, Ragnhild, Gal-Yam, Avishay, Ofek, Eran O., Perley, Daniel A., Filippenko, Alexei V., Kasliwal, Mansi M., Kulkarni, Shri R., Nugent, Peter E., Quimby, Robert M., Sullivan, Mark, Strothjohann, Nora Linn, Arcavi, Iair, Ben-Ami, Sagi, Bianco, Federica, Bloom, Joshua S., De, Kishalay, Fraser, Morgan, Fremling, Christoffer U., Horesh, Assaf, Johansson, Joel, Kelly, Patrick L., Knezevic, Sladjana, Maguire, Kate, Nyholm, Anders, Papadogiannakis, 2 Semeli, Petrushevska, Tanja, Rubin, Adam, Yan, Lin, Yang, Yi, Adams, Scott M., Bufano, Filomena, Clubb, Kelsey I., Foley, Ryan J., Green, Yoav, Harmanen, Jussi, Ho, Anna Y. Q., Hook, Isobel M., Hosseinzadeh, Griffin, Howell, D. Andrew, Kong, Albert K. H., Kotak, Rubina, Matheson, Thomas, McCully, Curtis, Milisavljevic, Dan, Pan, Yen-Chen, Poznanski, Dovi, Shivvers, Isaac, van Velzen, Sjoert
Several thousand core-collapse supernovae (CCSNe) of different flavors have been discovered so far. However, identifying their progenitors has remained an outstanding open question in astrophysics. Studies of SN host galaxies have proven to be powerf
Externí odkaz:
http://arxiv.org/abs/2008.05988
Autor:
Nyholm, Anders
A supernova (SN) is the explosive destruction of a star. Via a luminous outpouring of radiation, the SN can rival the brightness of its SN host galaxy for months or years. In the past decade, astronomical surveys regularly observing the sky to deep l
Externí odkaz:
http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-147289
Autor:
Arcavi, Iair, Howell, D. Andrew, Kasen, Daniel, Bildsten, Lars, Hosseinzadeh, Griffin, McCully, Curtis, Wong, Zheng Chuen, Katz, Sarah Rebekah, Gal-Yam, Avishay, Sollerman, Jesper, Taddia, Francesco, Leloudas, Giorgos, Fremling, Christoffer, Nugent, Peter E., Horesh, Assaf, Mooley, Kunal, Rumsey, Clare, Cenko, S. Bradley, Graham, Melissa L., Perley, Daniel A., Nakar, Ehud, Shaviv, Nir J., Bromberg, Omer, Shen, Ken J., Ofek, Eran O., Cao, Yi, Wang, Xiaofeng, Huang, Fang, Rui, Liming, Zhang, Tianmeng, Li, Wenxiong, Li, Zhitong, Zhang, Jujia, Valenti, Stefano, Guevel, David, Shappee, Benjamin, Kochanek, Christopher S., Holoien, Thomas W. -S., Filippenko, Alexei V., Fender, Rob, Nyholm, Anders, Yaron, Ofer, Kasliwal, Mansi M., Sullivan, Mark, Blagorodnova, Nadja, Walters, Richard S., Lunnan, Ragnhild, Khazov, Danny, Andreoni, Igor, Laher, Russ R., Konidaris, Nick, Wozniak, Przemek, Bue, Brian
Every supernova hitherto observed has been considered to be the terminal explosion of a star. Moreover, all supernovae with absorption lines in their spectra show those lines decreasing in velocity over time, as the ejecta expand and thin, revealing
Externí odkaz:
http://arxiv.org/abs/1711.02671
Autor:
Villarroel, Beatriz, Nyholm, Anders, Karlsson, Torgny, Comerón, Sébastien, Korn, Andreas, Sollerman, Jesper, Zackrisson, Erik
Active Galactic Nuclei (AGN) are extremely powerful cosmic objects, driven by accretion of hot gas upon super-massive black holes. The zoo of AGN classes are divided into two major groups, with Type-1 AGN displaying broad Balmer emission lines and Ty
Externí odkaz:
http://arxiv.org/abs/1701.08647
Autor:
Schulze, Steve, Yaron, Ofer, Sollerman, Jesper, Leloudas, Giorgos, Gal, Amit, Wright, Angus H., Lunnan, Ragnhild, Gal-Yam, Avishay, Ofek, Eran O., Perley, Daniel A., Filippenko, Alexei V., Kasliwal, Mansi M., Kulkarni, Shri R., Nugent, Peter E., Quimby, Robert M., Sullivan, Mark, Strothjohann, Nora Linn, Arcavi, Iair, Ben-Ami, Sagi, Bianco, Federica, Bloom, Joshua S., De, Kishalay, Fraser, Morgan, Fremling, Christoffer U., Horesh, Assaf, Johansson, Joel, Kelly, Patrick L., Knezevic, Sladjana, Maguire, Kate, Nyholm, Anders, Papadogiannakis, 2 Semeli, Petrushevska, Tanja, Rubin, Adam, Yan, Lin, Yang, Yi, Adams, Scott M., Bufano, Filomena, Clubb, Kelsey I., Foley, Ryan J., Green, Yoav, Harmanen, Jussi, Ho, Anna Y. Q., Hook, Isobel M., Hosseinzadeh, Griffin, Howell, D. Andrew, Kong, Albert K. H., Kotak, Rubina, Matheson, Thomas, McCully, Curtis, Milisavljevic, Dan, Pan, Yen-Chen, Poznanski, Dovi, Shivvers, Isaac, van Velzen, Sjoert
Several thousand core-collapse supernovae (CCSNe) of different flavors have been discovered so far. However, identifying their progenitors has remained an outstanding open question in astrophysics. Studies of SN host galaxies have proven to be powerf
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9d27e1fb95ddc13e0ce6747e487c96d7
https://eprints.soton.ac.uk/453990/
https://eprints.soton.ac.uk/453990/
Akademický článek
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Autor:
Nyholm, Anders
Some stars cease to be in a bright and destructive display called a supernova. This thesis explores what we can learn about supernovae (SNe) by studying their immediate surroundings, and what the SNe can teach us about their environments. The work pr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::9ac2232b46e798d0b2feeb73f0896a2f
http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-171451
http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-171451
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.