Zobrazeno 1 - 10
of 111
pro vyhledávání: '"Ustamujić A"'
Autor:
Elbisa Ustamujić
Publikováno v:
Društvene i Humanističke Studije, Vol 9, Iss 1(25), Pp 57-64 (2024)
The paper analyzes the novel Most and the essay Iskaz poneblja written on the occasion of the novel Grozdana's giggle by Hamza Hume from Jasmina Musabegović's oeuvre. In these texts, the writer expressed her attachment to the South - Herzegovina, Mo
Externí odkaz:
https://doaj.org/article/aee04629899e49e7b270099f60a46df7
Autor:
Prisinzano, L., Bonito, R., Mazzi, A., Damiani, F., Ustamujic, S., Yoachim, P., Street, R., Guarcello, M. G., Venuti, L., Clarkson, W., Jones, L., Girardi, L.
A complete map of the youngest stellar populations of the Milky Way in the era of all-sky surveys, is one of the most challenging goals in modern astrophysics. The characterisation of the youngest stellar component is crucial not only for a global ov
Externí odkaz:
http://arxiv.org/abs/2302.08604
Autor:
Bonito, R., Venuti, L., Ustamujic, S., Yoachim, P., Street, R. A., Prisinzano, L., Hartigan, P., Guarcello, M. G., Stassun, K. G., Giannini, T., Feigelson, E. D., Garatti, A. Caratti o, Orlando, S., Clarkson, W. I., McGehee, P., Bellm, E. C., Gizis, J. E.
Vera C. Rubin Observatory, through the Legacy Survey of Space and Time (LSST), will allow us to derive a panchromatic view of variability in young stellar objects (YSOs) across all relevant timescales. Indeed, both short-term variability (on timescal
Externí odkaz:
http://arxiv.org/abs/2302.00897
The complexity of the data generated by (magneto)-hydrodynamic (HD/MHD) simulations requires advanced tools for their analysis and visualization. The dramatic improvements in virtual reality (VR) technologies have inspired us to seek the long-term go
Externí odkaz:
http://arxiv.org/abs/2301.11334
Autor:
Breivik, Katelyn, Connolly, Andrew J., Ford, K. E. Saavik, Jurić, Mario, Mandelbaum, Rachel, Miller, Adam A., Norman, Dara, Olsen, Knut, O'Mullane, William, Price-Whelan, Adrian, Sacco, Timothy, Sokoloski, J. L., Villar, Ashley, Acquaviva, Viviana, Ahumada, Tomas, AlSayyad, Yusra, Alves, Catarina S., Andreoni, Igor, Anguita, Timo, Best, Henry J., Bianco, Federica B., Bonito, Rosaria, Bradshaw, Andrew, Burke, Colin J., de Campos, Andresa Rodrigues, Cantiello, Matteo, Caplar, Neven, Chandler, Colin Orion, Chan, James, da Costa, Luiz Nicolaci, Danieli, Shany, Davenport, James R. A., Fabbian, Giulio, Fagin, Joshua, Gagliano, Alexander, Gall, Christa, Camargo, Nicolás Garavito, Gawiser, Eric, Gezari, Suvi, Gomboc, Andreja, Gonzalez-Morales, Alma X., Graham, Matthew J., Gschwend, Julia, Guy, Leanne P., Holman, Matthew J., Hsieh, Henry H., Hundertmark, Markus, Ilić, Dragana, Ishida, Emille E. O., Jurkić, Tomislav, Kannawadi, Arun, Kosakowski, Alekzander, Kovačević, Andjelka B., Kubica, Jeremy, Lanusse, François, Lazar, Ilin, Levine, W. Garrett, Li, Xiaolong, Lu, Jing, Luna, Gerardo Juan Manuel, Mahabal, Ashish A., Malz, Alex I., Mao, Yao-Yuan, Medan, Ilija, Moeyens, Joachim, Nikolić, Mladen, Nikutta, Robert, O'Dowd, Matt, Olsen, Charlotte, Pearson, Sarah, Pedraza, Ilhuiyolitzin Villicana, Popinchalk, Mark, Popović, Luka C., Pritchard, Tyler A., Quint, Bruno C., Radović, Viktor, Ragosta, Fabio, Riccio, Gabriele, Riley, Alexander H., Rożek, Agata, Sánchez-Sáez, Paula, Sarro, Luis M., Saunders, Clare, Savić, Đorđe V., Schmidt, Samuel, Scott, Adam, Shirley, Raphael, Smotherman, Hayden R., Stetzler, Steven, Storey-Fisher, Kate, Street, Rachel A., Trilling, David E., Tsapras, Yiannis, Ustamujic, Sabina, van Velzen, Sjoert, Vázquez-Mata, José Antonio, Venuti, Laura, Wyatt, Samuel, Yu, Weixiang, Zabludoff, Ann
The Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) dataset will dramatically alter our understanding of the Universe, from the origins of the Solar System to the nature of dark matter and dark energy. Much of this research will depe
Externí odkaz:
http://arxiv.org/abs/2208.02781
Low-mass pre-main sequence (PMS) stars are strong X-ray sources, because they possess hot corona like their older main-sequence counterparts. Unique to young stars, however, are X-rays from accretion and outflows, and both processes are of pivotal im
Externí odkaz:
http://arxiv.org/abs/2207.06886
Autor:
Cosentino, G., Jiménez-Serra, I., Tan, J. C., Henshaw, J. D., Barnes, A. T., Law, C. -Y., Zeng, S., Fontani, F., Caselli, P., Viti, S., Zahorecz, S., Rico-Villas, F., Megías, A., Miceli, M., Orlando, S., Ustamujic, S., Greco, E., Peres, G., Bocchino, F., Fedriani, R., Gorai, P., Testi, L., Martín-Pintado, J.
Supernova remnants (SNRs) contribute to regulate the star formation efficiency and evolution of galaxies. As they expand into the interstellar medium (ISM), they transfer vast amounts of energy and momentum that displace, compress and heat the surrou
Externí odkaz:
http://arxiv.org/abs/2201.03008
Autor:
Ustamujic, S., Orlando, S., Miceli, M., Bocchino, F., Limongi, M., Chieffi, A., Trigilio, C., Umana, G., Bufano, F., Ingallinera, A., Peres, G.
Publikováno v:
A&A 654, A167 (2021)
LBVs are massive evolved stars that suffer sporadic and violent mass-loss events. They have been proposed as the progenitors of some core-collapse SNe, but this idea is still debated due to the lack of direct evidence. Since SNRs can carry in their m
Externí odkaz:
http://arxiv.org/abs/2108.01951
Autor:
Orlando, S., Miceli, M., Ustamujic, S., Tutone, A., Greco, E., Petruk, O., Bocchino, F., Peres, G.
According to the most popular model for the origin of cosmic rays (CRs), supernova remnants (SNRs) are the site where CRs are accelerated. Observations across the electromagnetic spectrum support this picture through the detection of non-thermal emis
Externí odkaz:
http://arxiv.org/abs/2012.13394
Publikováno v:
A&A 649, A14 (2021)
The morphology and the distribution of material observed in SNRs reflect the interaction of the SN blast wave with the ambient environment, the physical processes associated with the SN explosion and the internal structure of the progenitor star. IC
Externí odkaz:
http://arxiv.org/abs/2012.08017