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pro vyhledávání: '"elliptical and lenticular, cD [Galaxies]"'
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Autor:
Pablo M Galán-de Anta, Pedro R Capelo, Eugene Vasiliev, Massimo Dotti, Marc Sarzi, Enrico Maria Corsini, Lorenzo Morelli
Publikováno v:
Galán-De Anta, P M, Capelo, P R, Vasiliev, E, Dotti, M, Sarzi, M, Corsini, E M & Morelli, L 2023, ' The fragility of thin discs in galaxies-II. Thin discs as tracers of the assembly history of galaxies ', Monthly Notices of the Royal Astronomical Society, vol. 523, no. 3, pp. 3939-3948 . https://doi.org/10.1093/mnras/stad1593
Thin galactic discs and nuclear stellar discs (NSDs) are fragile structures that can be easily disturbed by merger events. By studying the age of the stellar populations in present-day discs, we can learn about the assembly history of galaxies and pl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5fa2c5b7cb46da4532ca7d086e2f2d15
https://pure.qub.ac.uk/en/publications/4a047752-2799-4bd0-859c-73bb83d686f9
https://pure.qub.ac.uk/en/publications/4a047752-2799-4bd0-859c-73bb83d686f9
Autor:
Timothy A Davis, Jindra Gensior, Martin Bureau, Michele Cappellari, Woorak Choi, Jacob S Elford, J M Diederik Kruijssen, Federico Lelli, Fu-Heng Liang, Lijie Liu, Ilaria Ruffa, Toshiki Saito, Marc Sarzi, Andreas Schruba, Thomas G Williams
Publikováno v:
Davis, T A, Gensior, J, Bureau, M, Cappellari, M, Choi, W, Elford, J S, Kruijssen, J M D, Lelli, F, Liang, F-H, Liu, L, Ruffa, I, Saito, T, Sarzi, M, Schruba, A & Williams, T G 2022, ' WISDOM Project-X. The morphology of the molecular ISM in galaxy centres and its dependence on galaxy structure ', Monthly Notices of the Royal Astronomical Society, vol. 512, no. 1, pp. 1522-1540 . https://doi.org/10.1093/mnras/stac600
Davis, T A, Gensior, J, Bureau, M, Cappellari, M, Choi, W, Elford, J S, Kruijssen, J M D, Lelli, F, Liang, F-H, Liu, L, Ruffa, I, Saito, T, Sarzi, M, Schruba, A & Williams, T G 2022, ' WISDOM Project-X. The morphology of the molecular ISM in galaxy centres and its dependence on galaxy structure ', Monthly Notices of the Royal Astronomical Society, vol. 512, no. 1, pp. 1522–1540 . https://doi.org/10.1093/mnras/stac600
Davis, T A, Gensior, J, Bureau, M, Cappellari, M, Choi, W, Elford, J S, Kruijssen, J M D, Lelli, F, Liang, F-H, Liu, L, Ruffa, I, Saito, T, Sarzi, M, Schruba, A & Williams, T G 2022, ' WISDOM Project-X. The morphology of the molecular ISM in galaxy centres and its dependence on galaxy structure ', Monthly Notices of the Royal Astronomical Society, vol. 512, no. 1, pp. 1522–1540 . https://doi.org/10.1093/mnras/stac600
We use high-resolution maps of the molecular interstellar medium (ISM) in the centres of eighty-six nearby galaxies from the millimetre-Wave Interferometric Survey of Dark Object Masses (WISDOM) and Physics at High Angular Resolution in Nearby Galaxi
Autor:
Pablo M Galán-de Anta, Eugene Vasiliev, Marc Sarzi, Massimo Dotti, Pedro R Capelo, Andrea Incatasciato, Lorenzo Posti, Lorenzo Morelli, Enrico Maria Corsini
Publikováno v:
Galán-De Anta, P M, Vasiliev, E, Sarzi, M, Dotti, M, Capelo, P R, Incatasciato, A, Posti, L, Morelli, L & Corsini, E M 2023, ' The fragility of thin discs in galaxies – I. Building tailored N-body galaxy models ', Monthly Notices of the Royal Astronomical Society, vol. 520, no. 3, pp. 4490-4501 . https://doi.org/10.1093/mnras/stad419
Thin stellar discs on both galactic and nuclear, sub-kpc scales are believed to be fragile structures that would be easily destroyed in major mergers. In turn, this makes the age-dating of their stellar populations a useful diagnostics for the assemb
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8636c290417fb87937b9e249e41b03e8
Autor:
Kaipper, André Luiz Pompeo
Publikováno v:
Biblioteca Digital de Teses e Dissertações do UFSM
Universidade Federal de Santa Maria (UFSM)
instacron:UFSM
Universidade Federal de Santa Maria (UFSM)
instacron:UFSM
Coordenação de Aperfeiçoamento de Pessoal de Nível Superior - CAPES In this work, we revisit the problem of morphological classification of BCG galaxies, in order to identify the characteristic signatures of cD-class galaxies. For this, we analyz
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3056::49017aad36dabdc1cc6a3d5fbd9b4948
http://repositorio.ufsm.br/handle/1/26645
http://repositorio.ufsm.br/handle/1/26645
Autor:
Watkins, A. E. (A. E.), Salo, H. (H.), Laurikainen, E. (E.), Díaz-García, S. (S.), Comerón, S. (S.), Janz, J. (J.), Su, A. H. (A. H.), Buta, R. (R.), Athanassoula, E. (E.), Bosma, A. (A.), Ho, L. C. (L. C.), Holwerda, B. W. (B. W.), Kim, T. (T.), Knapen, J. H. (J. H.), Laine, S. (S.), Menéndez-Delmestre, K. (K.), Peletier, R. F. (R. F.), Sheth, K. (K.), Zaritsky, D. (D.)
Context.: The Spitzer Survey of Stellar Structure in Galaxies (S⁴G) is a detailed study of over 2300 nearby galaxies in the near-infrared (NIR), which has been critical to our understanding of the detailed structures of nearby galaxies. Because the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::4f548c1df429bc1829952eb0426ffeb9
https://resolver.caltech.edu/CaltechAUTHORS:20220414-26705000
https://resolver.caltech.edu/CaltechAUTHORS:20220414-26705000
In many investigations involving accretion on a central point mass, ranging from observational studies to cosmological simulations, including semi-analytical modelling, the classical Bondi accretion theory is the standard tool widely adopted. Previou
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3012df21c0dad7296af1084d5d616821
http://arxiv.org/abs/2203.05050
http://arxiv.org/abs/2203.05050
Autor:
Chiara Spiniello, Ignacio Trujillo, Stefano Cavuoti, C. Lidman, C. E. Petrillo, Massimo Brescia, Mario Radovich, Giuseppe D'Ago, F. La Barbera, N. Roy, M. A. Raj, Marilena Spavone, Aniello Grado, Giuseppe Longo, M. Capaccioli, Fedor Getman, Vincenzo Pota, Christian Wolf, G. A. Verdoes Kleijn, Chris Blake, D. Scognamiglio, Léon V. E. Koopmans, Karl Glazebrook, Shahab Joudaki, Konrad Kuijken, Giovanni Covone, C. Tortora, Nicola R. Napolitano
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 481(4), 4728-4752
Monthly Notices of the Royal Astronomical Society, 481(4), 4728-4752. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 481(4), 4728-4752
Monthly Notices of the Royal Astronomical Society, 481(4), 4728-4752. Oxford University Press
We present results from an ongoing investigation using the Kilo Degree Survey (KiDS) on the VLT Survey Telescope (VST) to provide a census of ultra-compact massive galaxies (UCMGs), defined as galaxies with stellar masses $M_{\rm \star} > 8 \times 10
Autor:
Capetti, A., Brienza, M., Balmaverde, B., Best, P. N., Baldi, R. D., Drabent, A., Gürkan, G., Rottgering, H. J. A., Tasse, C., Webster, B.
Publikováno v:
Capetti, A, Brienza, M, Balmaverde, B, Best, P N, Baldi, R D, Drabent, A, Gurkan, G, Rottgering, H J A, Tasse, C & Webster, B 2022, ' The LOFAR view of giant, early-type galaxies radio emission from active nuclei and star formation ', Astronomy and Astrophysics, vol. 660, A93, pp. 1-22 . https://doi.org/10.1051/0004-6361/202142911
Astronomy & Astrophysics, 660:A93
Astronomy & Astrophysics, 660:A93
We study the properties and the origin of the radio emission in the most luminous early-type galaxies (ETGs) in the nearby Universe (MK
Comment: Pre-proofs version - Accepted for publication in A&A
Comment: Pre-proofs version - Accepted for publication in A&A
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2cae59ac79b8bd77bed10a11a2890fef
Autor:
Junkai Zhang, Stijn Wuyts, Callum Witten, Charlotte R Avery, Lei Hao, Raman Sharma, Juntai Shen, Jun Toshikawa, Carolin Villforth
Publikováno v:
Zhang, J, Wuyts, S, Witten, C, Avery, C R, Hao, L, Sharma, R, Shen, J, Toshikawa, J & Villforth, C 2022, ' 3D intrinsic shapes of quiescent galaxies in observations and simulations ', Monthly Notices of the Royal Astronomical Society, vol. 513, no. 4, pp. 4814-4832 . https://doi.org/10.1093/mnras/stac1083
We study the intrinsic 3D shapes of quiescent galaxies over the last half of cosmic history based on their axial ratio distribution. To this end, we construct a sample of unprecedented size, exploiting multi-wavelength $u$-to-$K_s$ photometry from th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::81c52d1f74c10eb661d84e5f2b3aa492