Zobrazeno 1 - 10
of 288
pro vyhledávání: '"D Milisavljevic"'
Autor:
S Al Kharusi, S Y BenZvi, J S Bobowski, W Bonivento, V Brdar, T Brunner, E Caden, M Clark, A Coleiro, M Colomer-Molla, J I Crespo-Anadón, A Depoian, D Dornic, V Fischer, D Franco, W Fulgione, A Gallo Rosso, M Geske, S Griswold, M Gromov, D Haggard, A Habig, O Halim, A Higuera, R Hill, S Horiuchi, K Ishidoshiro, C Kato, E Katsavounidis, D Khaitan, J P Kneller, A Kopec, V Kulikovskiy, M Lai, M Lamoureux, R F Lang, H L Li, M Lincetto, C Lunardini, J Migenda, D Milisavljevic, M E McCarthy, E O Connor, E O Sullivan, G Pagliaroli, D Patel, R Peres, B W Pointon, J Qin, N Raj, A Renshaw, A Roeth, J Rumleskie, K Scholberg, A Sheshukov, T Sonley, M Strait, V Takhistov, I Tamborra, J Tseng, C D Tunnell, J Vasel, C F Vigorito, B Viren, C J Virtue, J S Wang, L J Wen, L Winslow, F L H Wolfs, X J Xu, Y Xu
Publikováno v:
New Journal of Physics, Vol 23, Iss 3, p 031201 (2021)
The next core-collapse supernova in the Milky Way or its satellites will represent a once-in-a-generation opportunity to obtain detailed information about the explosion of a star and provide significant scientific insight for a variety of fields beca
Externí odkaz:
https://doaj.org/article/6bbda9d6120c404bb8f2f3628555ad72
Autor:
J. Rho, S.-H. Park, R. Arendt, M. Matsuura, D. Milisavljevic, T. Temim, I. De Looze, W. P. Blair, A. Rest, O. Fox, A. P. Ravi, B.-C. Koo, M. Barlow, A. Burrows, R. Chevalier, G. Clayton, R. Fesen, C. Fransson, C. Fryer, H. L. Gomez, H.-T. Janka, F. Kirchschlager, J. M. Laming, S. Orlando, D. Patnaude, G. Pavlov, P. Plucinsky, B. Posselt, F. Priestley, J. Raymond, N. Sartorio, F. Schmidt, P. Slane, N. Smith, N. Sravan, J. Vink, K. Weil, J. Wheeler, S. C. Yoon
Publikováno v:
The Astrophysical Journal Letters, Vol 969, Iss 1, p L9 (2024)
We present JWST NIRCam (F356W and F444W filters) and MIRI (F770W) images and NIRSpec Integral Field Unit (IFU) spectroscopy of the young Galactic supernova remnant Cassiopeia A (Cas A) to probe the physical conditions for molecular CO formation and d
Externí odkaz:
https://doaj.org/article/016bc259901442d3a49e82bfea30349c
Autor:
Giulia Migliori, R. Margutti, B. D. Metzger, R. Chornock, C. Vignali, D. Brethauer, D. L. Coppejans, T. Maccarone, L. Rivera Sandoval, J. S. Bright, T. Laskar, D. Milisavljevic, E. Berger, A. J. Nayana
Publikováno v:
The Astrophysical Journal Letters, Vol 963, Iss 1, p L24 (2024)
We present the first deep X-ray observations of luminous fast blue optical transient (LFBOT) AT 2018cow at ∼3.7 yr since discovery, together with the reanalysis of the observation at δ t ∼ 220 days. X-ray emission is significantly detected at a
Externí odkaz:
https://doaj.org/article/00f566ea293e46778ab2f4f352b06703
Autor:
W. V. Jacobson-Galán, K. W. Davis, C. D. Kilpatrick, L. Dessart, R. Margutti, R. Chornock, R. J. Foley, P. Arunachalam, K. Auchettl, C. R. Bom, R. Cartier, D. A. Coulter, G. Dimitriadis, D. Dickinson, M. R. Drout, A. T. Gagliano, C. Gall, B. Garretson, L. Izzo, D. O. Jones, N. LeBaron, H.-Y. Miao, D. Milisavljevic, Y.-C. Pan, A. Rest, C. Rojas-Bravo, A. Santos, H. Sears, B. M. Subrayan, K. Taggart, S. Tinyanont
Publikováno v:
The Astrophysical Journal, Vol 972, Iss 2, p 177 (2024)
We present UV–optical–near-infrared observations and modeling of supernova (SN) 2024ggi, a type II supernova (SN II) located in NGC 3621 at 7.2 Mpc. Early-time (“flash”) spectroscopy of SN 2024ggi within +0.8 days of discovery shows emission
Externí odkaz:
https://doaj.org/article/e1c8f5ec08464919a5dfa4b5ef64d279
Autor:
S. Orlando, A. Wongwathanarat, H.-T. Janka, M. Miceli, S. Nagataki, M. Ono, F. Bocchino, J. Vink, D. Milisavljevic, D. J. Patnaude, G. Peres
Publikováno v:
Astronomy and Astrophysics, 666:A2. EDP Sciences
Observations of the SNR Cassiopeia A (Cas A) show asymmetries in the reverse shock that cannot be explained by models describing a remnant expanding through a spherically symmetric wind of the progenitor star. We investigate whether a past interactio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a6b943e2e3ce693212f3d82c26d0f0fc
https://hdl.handle.net/10447/573826
https://hdl.handle.net/10447/573826
Akademický článek
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Akademický článek
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Akademický článek
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Autor:
Maria Niculescu-Duvaz, M J Barlow, A Bevan, R Wesson, D Milisavljevic, I De Looze, G C Clayton, K Krafton, M Matsuura, R Brady
Publikováno v:
Monthly Notices of the Royal Astronomical Society
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Modelling the red-blue asymmetries seen in the broad emission lines of core-collapse supernovae (CCSNe) is a powerful technique to quantify total dust mass formed in the ejecta at late times ($>5$ years after outburst) when ejecta dust temperatures b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ec7930019b461ece6e31f667b17acb94
https://orca.cardiff.ac.uk/id/eprint/152108/1/stac1626.pdf
https://orca.cardiff.ac.uk/id/eprint/152108/1/stac1626.pdf
Autor:
W. V. Jacobson-Galán, P. Venkatraman, R. Margutti, D. Khatami, G. Terreran, R. J. Foley, R. Angulo, C. R. Angus, K. Auchettl, P. K. Blanchard, A. Bobrick, J. S. Bright, D. Brout, K. C. Chambers, C. D. Couch, D. A. Coulter, K. Clever, K. W. Davis, T. J. L. de Boer, L. DeMarchi, S. A. Dodd, D. O. Jones, J. Johnson, C. D. Kilpatrick, N. Khetan, Z. Lai, D. Langeroodi, C.-C. Lin, E. A. Magnier, D. Milisavljevic, H. B. Perets, J. D. R. Pierel, J. Raymond, S. Rest, A. Rest, R. Ridden-Harper, K. J. Shen, M. R. Siebert, C. Smith, K. Taggart, S. Tinyanont, F. Valdes, V. A. Villar, Q. Wang, S. K. Yadavalli, Y. Zenati, A. Zenteno
Publikováno v:
Jacobson-Galan, W V, Venkatraman, P, Margutti, R, Khatami, D, Terreran, G, Foley, R J, Angulo, R, Angus, C R, Auchettl, K, Blanchard, P K, Bobrick, A, Bright, J S, Brout, D, Chambers, K C, Couch, C D, Coulter, D A, Clever, K, Davis, K W, de Boer, T J L, DeMarchi, L, Dodd, S A, Jones, D O, Johnson, J, Kilpatrick, C D, Khetan, N, Lai, Z, Langeroodi, D, Lin, C-C, Magnier, E A, Milisavljevic, D, Perets, H B, Pierel, J D R, Raymond, J, Rest, S, Rest, A, Ridden-Harper, R, Shen, K J, Siebert, M R, Smith, C, Taggart, K, Tinyanont, S, Valdes, F, Villar, V A, Wang, Q, Yadavalli, S K, Zenati, Y & Zenteno, A 2022, ' The Circumstellar Environments of Double-peaked, Calcium-strong Transients 2021gno and 2021inl ', Astrophysical Journal, vol. 932, no. 1, 58 . https://doi.org/10.3847/1538-4357/ac67dc
We present panchromatic observations and modeling of calcium-strong supernovae (SNe) 2021gno in the star-forming host-galaxy NGC 4165 and 2021inl in the outskirts of elliptical galaxy NGC 4923, both monitored through the Young Supernova Experiment tr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ba22b71685953059d46ebd8b20f5d94b
https://curis.ku.dk/ws/files/315472935/Jacobson_Gal_n_2022_ApJ_932_58.pdf
https://curis.ku.dk/ws/files/315472935/Jacobson_Gal_n_2022_ApJ_932_58.pdf