Zobrazeno 1 - 10
of 31
pro vyhledávání: '"Spavone, M."'
Autor:
Maccagni, F. M., Ruffa, I., Loni, A., Prandoni, I., Ragusa, R., Kleiner, D., Serra, P., Iodice, E., Spavone, M.
We present Australia Compact Telescope Array (ATCA) 21-cm observations of the nearby low-excitation radio galaxy (LERG) NGC 3100. This is the brightest galaxy of a loose group and hosts a young ($\sim 2$ Myr) radio source. The ATCA observations revea
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9c2c9fe20dffe62db0e1c561dc297dfc
Autor:
Napolitano, N. R., Gatto, M., Spiniello, C., Cantiello, M., Hilker, M., Arnaboldi, M., Tortora, C., Chaturvedi, A., D'Abrusco, R., Li, R., Paolillo, M., Peletier, R., Saifollahi, T., Spavone, M., Venhola, A., Pota, V., Capaccioli, M., Longo, G.
Publikováno v:
Astronomy and astrophysics, 657:A94. EDP Sciences
The COld STream finder Algorithm (COSTA) is a novel algorithm to find streams in the phase space of planetary nebulae (PNe) and globular cluster (GCs) populations. COSTA isolates groups of particles with small velocity dispersion, using an iterative
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d00d15319a161f64607373bd4a30a904
http://urn.fi/urn:nbn:fi-fe2023030830678
http://urn.fi/urn:nbn:fi-fe2023030830678
Autor:
Martin, G., Bazkiaei, A. E., Spavone, M., Iodice, E., Mihos, J. C., Montes, M., Benavides, J. A., Brough, S., Carlin, J. L., Collins, C. A., Duc, P. A., Gómez, F. A., Galaz, G., Hernández-Toledo, H. M., Jackson, R. A., Kaviraj, S., Knapen, J. H., Martínez-Lombilla, C., McGee, S., O'Ryan, D., Prole, D. J., Rich, R. M., Román, J., Shah, E. A., Starkenburg, T. K., Watkins, A. E., Zaritsky, D., Laigle, C., Pichon, C., Armus, L., Bianconi, M., Buitrago, F., Busá, I., Davis, F., Demarco, R., Desmons, A., García, P., Graham, A. W., Holwerda, B., Hon, D. S. -H., Khalid, A., Klehammer, J., Klutse, D. Y., Lazar, I., Nair, P., Noakes-Kettel, E. A., Rutkowski, M., Saha, K., Sahu, N., Sola, E., Vázquez-Mata, J. A., Vera-Casanova, A., Yoon, I.
Tidal features in the outskirts of galaxies yield unique information about their past interactions and are a key prediction of the hierarchical structure formation paradigm. The Vera C. Rubin Observatory is poised to deliver deep observations for pot
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d0da1ea1cd081845e09f4d44466ac1e7
http://arxiv.org/abs/2203.07675
http://arxiv.org/abs/2203.07675
Autor:
Rampazzo, R., Mazzei, P., Marino, A., Bianchi, L., Postma, J., Ragusa, R., Spavone, M., Iodice, E., Ciroi, S., Held, E. V.
We are investigating the SF in galaxies of the actively evolving Dorado group where signatures of interactions and merging events are revealed by optical and radio observations in both ETGs and LTGs. Our previous Ha+[NII] study, probing ~10 Myrs time
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9d36d47c8f40760c7b7d8c2ebcd89200
Autor:
Gatto, M., Ripepi, V., Bellazzini, M., Dall'Ora, M., Tosi, M., Tortora, C., Cignoni, M., Cioni, M. -R. L., Cusano, F., Longo, G., Marconi, M., Musella, I., Schipani, P., Spavone, M.
We present FORS2@VLT follow-up photometry of YMCA-1, a recently discovered stellar system located 13\degr~from the Large Magellanic Cloud (LMC) center. The deep color-magnitude diagram (CMD) reveals a well-defined main sequence (MS) and a handful of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c0298bbccfebbfb90756710a3f2458c7
We present the first data release (DR1) of the VST Early-type GAlaxy Survey (VEGAS). This is a deep multi-band (u'g'r'i') imaging survey, carried out with the ESO VLT Survey Telescope (VST). To date, using about 90% of the total observing time, VEGAS
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d549cc6197630c47231470c33bf7b15b
Autor:
Riccio, G., Paolillo, M., D'Abrusco, R., Cantiello, M., Jin, X., Li, Z., Venhola, A., D'Ago, G., Puzia, Thomas H., Iodice, E., Pota, V., Napolitano, N., Hilker, M., Mieske, S., Spavone, M., Peletier, R., Eigenthaler, P., Bragaglia, A., Davies, M., Sills, A., Vesperini, E.
Publikováno v:
tar Clusters: From the Milky Way to the Early Universe: Proceedings of the International Astronomical Union, Volume 14, Symposium S351, 351, 151-154
The formation of Low mass X-ray binaries (LMXB) is favored within dense stellar systems such as Globular Clusters (GCs). The connection between LMXB and Globular Clusters has been extensively studied in the literature, but these studies have always b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d3e83307c32dedffff4887eb4d7aad75
https://research.rug.nl/en/publications/24921527-14bb-454a-8723-5b7b30ab320b
https://research.rug.nl/en/publications/24921527-14bb-454a-8723-5b7b30ab320b
Autor:
Tortora, C., Napolitano, N. R., Radovich, M., Spiniello, C., Hunt, L., Roy, N., Moscardini, L., Scognamiglio, D., Spavone, M., Brescia, M., Cavuoti, S., D`Ago, G., Longo, G., Bellagamba, F., Maturi, M., Roncarelli, M.
Relic galaxies are thought to be the progenitors of high-redshift red nuggets that for some reason missed the channels of size growth and evolved passively and undisturbed since the first star formation burst (at $z>2$). These local ultracompact old
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::83427568e5bfb2a3a8d2ba834debfdc5
Autor:
Spavone M., Capaccioli M., Cantiello M., Forbes D. A., Grado A., Iodice E., Limatola L., Napolitano N., Paolillo M., Puzia T. H., Raimondo G., Romanowsky A. J., Schipani P.
Publikováno v:
Astrophysics and Space Science Proceedings ISBN: 9783319193298
The VST-VEGAS project is aimed at observing and studying a rich sample of nearby early-type galaxies in order to systematically characterize their properties over a wide baseline of sizes and out to the faint outskirts where data are rather scarce so
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a9033a7163ae3d8734d2aedd5e3ceeb5
http://hdl.handle.net/11588/837451
http://hdl.handle.net/11588/837451
Autor:
Fiorentino, G., Bellazzini, M., Ciliegi, P., Chauvin, G., Douté, S., D'Orazi, V., Maiorano, E., Mannucci, F., Mapelli, M., Podio, L., Saracco, P., Spavone, M.
MAORY is the Adaptive Optic (AO) module that will be installed at the E-ELT at the first light of the telescope. It will provide two different types of AO correction, a very high correction over a small FoV (diameter ~10 arcsec, SCAO mode) and a mode
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::993d914cb2bb973aef2acf022a6824b4