Zobrazeno 1 - 10
of 510
pro vyhledávání: '"A. Omizzolo"'
Autor:
George, Koshy, Poggianti, B. M., Omizzolo, A., Vulcani, B., Côté, P., Postma, J., Smith, R., Jaffe, Y. L., Gullieuszik, M., Moretti, A., Subramaniam, A., Sreekumar, P., Ghosh, S. K., Tandon, S. N., Hutchings, J. B.
The assembly of galaxy clusters is understood to be a hierarchical process with a continuous accretion of galaxies over time, which increases the cluster size and mass. Late-type galaxies that fall into clusters can undergo ram-pressure stripping, fo
Externí odkaz:
http://arxiv.org/abs/2409.10586
Autor:
Luciano Luiz Alt, Amanda Delai Bortolini, Bruna Santin Andreis, Caroline Arais Schmidt, Giovana Rugeri, Maria Clara Tonini Pagliarin, Maria Eduarda Dupond Kindel, Maria Fernanda Almeida Costa, Nathália Lorenzoni Costa, Pedro Henrique Sarmento Dariz, Vinícius Grasseli Omizzolo
Publikováno v:
Journal of Mind and Medical Sciences, Vol 11, Iss 2, Pp 285-290 (2024)
Objectives. Although COVID-19 mainly affects the respiratory system, it can also cause neurological complications like memory impairment, which may be part of post-COVID-19 Syndrome. Identifying these impairments is challenging due to the lack of app
Externí odkaz:
https://doaj.org/article/5ddb31de700d4070ac2bdb3ff4d73bcc
Autor:
Vulcani, B., Poggianti, B. M., Gullieuszik, M., Moretti, A., Fritz, J., Bettoni, D., Facciolli, B., Fasano, G., Omizzolo, A.
Determining which between projected local density and distance from the cluster center plays a major role in regulating morphological fractions in clusters is a longstanding debate. Reaching a definitive answer will shed light on the main physical me
Externí odkaz:
http://arxiv.org/abs/2302.02376
Autor:
Gullieuszik, Marco, Giunchi, Eric, Poggianti, Bianca M., Moretti, Alessia, Scarlata, Claudia, Calzetti, Daniela, Werle, Ariel, Zanella, Anita, Radovich, Mario, Bellhouse, Callum, Bettoni, Daniela, Franchetto, Andrea, Fritz, Jacopo, Jaffé, Yara L., McGee, Sean, Mingozzi, Matilde, Omizzolo, Alessando, Tonnesen, Stephanie, Verheijen, Marc, Vulcani, Benedetta
Star-forming, H$\alpha$-emitting clumps are found embedded in the gaseous tails of galaxies undergoing intense ram-pressure stripping in galaxy clusters, so-called jellyfish galaxies. These clumps offer a unique opportunity to study star formation un
Externí odkaz:
http://arxiv.org/abs/2301.08279
Autor:
George, Koshy, Poggianti, B. M., Tomičić, Neven, Postma, J., Côté, P., Fritz, J., Ghosh, S. K., Gullieuszik, M., Hutchings, J. B., Moretti, A., Omizzolo, A., Radovich, M., Sreekumar, P., Subramaniam, A., Tandon, S. N., Vulcani, B.
Spiral galaxies undergo strong ram-pressure effects when they fall into the galaxy cluster potential. As a consequence, their gas is stripped to form extended tails within which star formation can happen, giving them the typical jellyfish appearance.
Externí odkaz:
http://arxiv.org/abs/2212.02423
Autor:
Auricelia de Aguiar Silva, Welingthon dos Santos Silva, Simone Regina Omizzolo, Francisco de Assis Carvalho de Almada
Publikováno v:
Revista de Estudos em Educação e Diversidade, Vol 5, Iss 12 (2024)
O presente artigo traz uma abordagem sobre a democratização na educação pública a partir das discussões acerca de gênero e inclusão na educação. Em que objetivamos refletir a democratização da escola pública como norteador das discussõe
Externí odkaz:
https://doaj.org/article/13d6c0bdc3a648919420d40065ab630b
Autor:
Moretti, A., Radovich, M., Poggianti, B. M., Vulcani, B., Gullieuszik, M., Werle, A., Bellhouse, C., Bacchini, C., Fritz, J., Soucail, G., Richard, J., Franchetto, A., Tomicic, N., Omizzolo, A.
Ram pressure stripping has been proven to be effective in shaping galaxy properties in dense environments at low redshift. The availability of MUSE observations of a sample of distant (z$\sim 0.3-0.5$) clusters has allowed to search for galaxies subj
Externí odkaz:
http://arxiv.org/abs/2111.04501
Autor:
Boutsia, K., Grazian, A., Fontanot, F., Giallongo, E., Menci, N., Calderone, G., Cristiani, S., D'Odorico, V., Cupani, G., Guarneri, F., Omizzolo, A.
Based on results by recent surveys, the number of bright quasars at redshifts z>3 is being constantly revised upwards. Current consensus is that at bright magnitudes ($M_{1450}\le -27$) the number densities of such sources could have been underestima
Externí odkaz:
http://arxiv.org/abs/2103.10446
Autor:
Boutsia, K., Grazian, A., Calderone, G., Cristiani, S., Cupani, G., Guarneri, F., Fontanot, F., Amorin, R., D'Odorico, V., Giallongo, E., Salvato, M., Omizzolo, A., Romano, M., Menci, N.
We present the results of the spectroscopic follow up of the QUBRICS survey. The selection method is based on a machine learning approach applied to photometric catalogs, covering an area of $\sim$ 12,400 deg$^2$ in the Southern Hemisphere. The spect
Externí odkaz:
http://arxiv.org/abs/2008.03865
Autor:
Gullieuszik, Marco, Poggianti, Bianca M., McGee, Sean L., Moretti, Alessia, Vulcani, Benedetta, Tonnesen, Stephanie, Roediger, Elke, Jaffé, Yara L., Fritz, Jacopo, Franchetto, Andrea, Omizzolo, Alessandro, Bettoni, Daniela, Radovich, Mario, Wolter, Anna
Using MUSE observations from the GASP survey, we study 54 galaxies undergoing ram-pressure stripping (RPS) spanning a wide range in galaxy mass and host cluster mass. We use this rich sample to study how the star formation rate (SFR) in the tails of
Externí odkaz:
http://arxiv.org/abs/2006.16032