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Autor:
Bianchin, Marina
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 The supermassive black holes at the centre of massive galaxies can influence their host evolution. During their active phase, the matter in the central parsecs of galaxies flows
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3056::71ef432f8b8e7ee8e4a73081de64458b
http://repositorio.ufsm.br/handle/1/26106
http://repositorio.ufsm.br/handle/1/26106
Publikováno v:
Wuyts, S & Schreiber, N M F 2020, ' Structure and dynamics of high-z galaxies ', Proceedings of the International Astronomical Union, vol. 14, no. S353, pp. 271-278 . https://doi.org/10.1017/S1743921319009293
HST and integral-field spectroscopic observations of star-forming galaxies at cosmic noon provide a view on the spatial distribution of stars, gas and dust, and probe gaseous motions revealing the central gravitational potential and local feedback pr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::46ea40170a47b13b905fc70a1c443db9
https://doi.org/10.1017/s1743921319009293
https://doi.org/10.1017/s1743921319009293
Autor:
F. van de Voort, Dimitri A. Gadotti, Mélanie Chevance, George J. Bendo, Marco Grossi, F. Pinna, Sébastien Viaene, I. De Looze, Paolo Serra, N. Zabel, Boris Nedelchev, Aku Venhola, Marc Sarzi, P. Tim de Zeeuw, Reynier Peletier, E. Maria Corsini, Enrica Iodice, Timothy A. Davis, Maarten Baes, J. M. Diederik Kruijssen, Catherine Vlahakis
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 496(2), 2155-2182. Oxford University Press
Monthly Notices of the Royal Astronomical Society
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Monthly Notices of the Royal Astronomical Society, 496(2), 2155-2182
Monthly Notices of the Royal Astronomical Society
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Monthly Notices of the Royal Astronomical Society, 496(2), 2155-2182
We combine data from ALMA and MUSE to study the resolved (~300 pc scale) star formation relation (star formation rate vs. molecular gas surface density) in cluster galaxies. Our sample consists of 9 Fornax cluster galaxies, including spirals, ellipti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3ef80a7c70ef0d9ccfa96473ecfbb8b4
http://hdl.handle.net/11577/3354673
http://hdl.handle.net/11577/3354673
Autor:
G. C. Jones, Dominik Riechers, Y. Fudamoto, Margherita Talia, Andreas L. Faisst, Miroslava Dessauges-Zavadsky, John D. Silverman, Peter Capak, G. Rodighiero, Mauro Giavalisco, S. Bardelli, Lin Yan, G. Zamorani, Livia Vallini, E. Zucca, Matthieu Béthermin, O. Le Fevre, Paolo Cassata, Brian C. Lemaux, Carlotta Gruppioni, D. Vergani, Y. Khusanova, Michele Ginolfi, Roberto Maiolino, Francesca Pozzi, F. Loiacono, Anton M. Koekemoer, Daniel Schaerer, Edo Ibar, Médéric Boquien, Andrea Cimatti, Pascal Oesch
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters
Monthly Notices of the Royal Astronomical Society: Letters, 2020, 491, pp.L18-L23. ⟨10.1093/mnrasl/slz154⟩
Monthly Notices of the Royal Astronomical Society: Letters, 491(1), L18-L23
Monthly Notices of the Royal Astronomical Society: Letters, 2020, 491, pp.L18-L23. ⟨10.1093/mnrasl/slz154⟩
Monthly Notices of the Royal Astronomical Society: Letters, 491(1), L18-L23
We report the detection of [CII]158um emission from a system of three closely-separated sources in the COSMOS field at z~4.56, as part of the ALMA Large Program to INvestigate CII at Early times (ALPINE). The two dominant sources are closely associat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::49397c64b448f01fb7a32d5bd88a5959
https://resolver.caltech.edu/CaltechAUTHORS:20191002-135305171
https://resolver.caltech.edu/CaltechAUTHORS:20191002-135305171
Publikováno v:
Armitage, T, Kay, S & Barnes, D 2019, ' An application of machine learning techniques to galaxy cluster mass estimation using the MACSIS simulations ', Monthly Notices of the Royal Astronomical Society, vol. 484, no. 2, pp. 1526-1537 . https://doi.org/10.1093/mnras/stz039
Machine learning (ML) techniques, in particular supervised regression algorithms, are a promising new way to use multiple observables to predict a cluster's mass or other key features. To investigate this approach we use the \textsc{MACSIS} sample of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e2531f30ee13b9887af5c2c76cc4e0bd
https://pure.manchester.ac.uk/ws/files/85597667/Proj3Main.pdf
https://pure.manchester.ac.uk/ws/files/85597667/Proj3Main.pdf
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Many active galactic nuclei (AGN) and particularly narrow-line Seyfert 1 (NLS1) galaxies, usually exhibit blueshifts and blue wings in several emission lines, which are mainly associated with outflows and strong winds. In order to study the radial ve
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f574786dc2560d8362c9740c89681c14
https://www.aanda.org/10.1051/0004-6361/201731557
https://www.aanda.org/10.1051/0004-6361/201731557
Autor:
Barrera-Ballesteros, J. K., Garc��a-Lorenzo, B., Falc��n-Barroso, J., van de Ven, G., Lyubenova, M., Wild, V., M��ndez-Abreu, J., S��nchez, S. F., Marquez, I., Masegosa, J., Monreal-Ibero, A., Ziegler, B., del Olmo, A., Verdes-Montenegro, L., Garc��a-Benito, R., Husemann, B., Mast, D., Kehrig, C., Iglesias-Paramo, J., Marino, R. A., Aguerri, J. A. L., Walcher, C. J., V��lchez, J. M., Bomans, D. J., Cortijo-Ferrero, C., Delgado, R. M. Gonz��lez, Bland-Hawthorn, J., McIntosh, D. H., Bekeraite, Simona, Collaboration, the CALIFA
Publikováno v:
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Astronomy and astrophysics, 582:A21. EDP Sciences
Digital.CSIC. Repositorio Institucional del CSIC
instname
E-Prints Complutense. Archivo Institucional de la UCM
Universidad Complutense de Madrid
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Astronomy and astrophysics, 582:A21. EDP Sciences
Digital.CSIC. Repositorio Institucional del CSIC
instname
E-Prints Complutense. Archivo Institucional de la UCM
© 2015 ESO. We present spatially resolved stellar and/or ionized gas kinematic properties for a sample of 103 interacting galaxies, tracing all merger stages: close companions, pairs with morphological signatures of interaction, and coalesced merger
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ad6c2417cc99b3503538b7149b730711
https://doi.org/10.1051/0004-6361/201424935
https://doi.org/10.1051/0004-6361/201424935
Publikováno v:
Biblos-e Archivo. Repositorio Institucional de la UAM
instname
Monthly Notices of the Royal Astronomical Society, 449 (2)
Monthly Notices of the Royal Astronomical Society
Biblos-e Archivo: Repositorio Institucional de la UAM
Universidad Autónoma de Madrid
instname
Monthly Notices of the Royal Astronomical Society, 449 (2)
Monthly Notices of the Royal Astronomical Society
Biblos-e Archivo: Repositorio Institucional de la UAM
Universidad Autónoma de Madrid
Monthly Notices of the Royal Astronomical Society, 449 (2)
ISSN:0035-8711
ISSN:1365-2966
ISSN:1365-8711
ISSN:0035-8711
ISSN:1365-2966
ISSN:1365-8711
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5a5c337e576a8f43776ba220ee49882c
Autor:
Riffel, Rogemar André, Storchi-Bergmann, Thaisa, Winge, Claudia, McGregor, Peter J., Beck, Tracy, Schmitt, Henrique Roberto
Publikováno v:
Repositório Institucional da UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
We present 2D stellar and gaseous kinematics of the inner ~ 130×180 pc² of the Narrow-Line Seyfert 1 galaxy NGC4051 at a sampling of 4.5 pc, from near-infrared K-band spectroscopic observations obtained with the Gemini’s Near-infrared Integral Fi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3056::3b6f13411e81e6a62f12f3f3a37f1045