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pro vyhledávání: '"INDIVIDUAL GALAXIES"'
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Publikováno v:
Вісник Астрономічної школи, Vol 14, Iss 2, Pp 81-86 (2018)
The study of radiation of the interacting galaxies in different ranges enables to identify various processes occurring in them. The most active processes (such as star birth, material accretion onto the black holes, burster flashes, etc.) cause the a
Externí odkaz:
https://doaj.org/article/7451b170894849329dd8500808ef300c
Autor:
Sinenhlanhla P. Sikhosana, Kenda Knowles, C. H. Ishwara-Chandra, Matt Hilton, Kavilan Moodley, Neeraj Gupta
Publikováno v:
Galaxies, Vol 9, Iss 4, p 117 (2021)
Low frequency radio observations of galaxy clusters are a useful probe of the non-thermal intracluster medium (ICM), through observations of diffuse radio emission such as radio halos and relics. Current formation theories cannot fully account for so
Externí odkaz:
https://doaj.org/article/11563aba5a0148fda2dd688774e27e7a
Autor:
B. S. Frank, Lourdes Verdes-Montenegro, Russ Taylor, Wanga Mulaudzi, Natasha Maddox, Kelley M. Hess, N. J. Adams, Matt J. Jarvis, Shilpa Ranchod, Madalina Tudorache, Tariq Blecher, Rebecca A. A. Bowler, Jordan D. Collier, Anastasia A. Ponomareva, Roger Deane, Marcin Glowacki
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 506(2), 2753-2765. Oxford University Press
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC. Repositorio Institucional del CSIC
instname
We present the serendipitous discovery of a galaxy group in the XMM-LSS field with MIGHTEE Early Science observations. 20 galaxies are detected in H i in this z ∼0.044 group, with a 3σ column density sensitivity of NHI = 1.6 × 1020 cm-2. This gro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::deeaf69556e1eab67ea307186e2ad54f
https://doi.org/10.1093/mnras/stab1817
https://doi.org/10.1093/mnras/stab1817
Autor:
Carsten Henkel, Serena Viti, A. Fuente, Nanase Harada, M. Scourfield, Francoise Combes, Amélie Saintonge, Susanne Aalto, A. Alonso-Herrero, Sergio Martín, Shuro Takano, Kotaro Kohno, M. Krips, A. Usero, Santiago García-Burillo, Taku Nakajima, P. van der Werf
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 496(4), 5308-5329
Digital.CSIC. Repositorio Institucional del CSIC
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Universidad de Alicante (UA)
Instituto Nacional de Técnica Aeroespacial (INTA)
Digital.CSIC. Repositorio Institucional del CSIC
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Universidad de Alicante (UA)
Instituto Nacional de Técnica Aeroespacial (INTA)
We present results from Atacama Large Millimeter/submillimeter Array (ALMA) observations of CS from the nearby galaxy NGC 1068 ($\sim14$ Mpc). This Seyfert 2 barred galaxy possesses a circumnuclear disc (CND, $r\sim200$ pc) and a starburst ring (SB r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6e680f28838f21131daed3112ce43824
https://doi.org/10.1093/mnras/staa1891
https://doi.org/10.1093/mnras/staa1891
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 494, 4, pp. 5207-5229
Monthly Notices of the Royal Astronomical Society, 494, 5207-5229
Musoke, G, Young, A J, Molnar, S M & Birkinshaw, M 2020, ' Numerical simulations of colliding jets in an external wind : application to 3C 75 ', Monthly Notices of the Royal Astronomical Society, vol. 494, no. 4, staa1071, pp. 5207-5229 . https://doi.org/10.1093/mnras/staa1071
Monthly Notices of the Royal Astronomical Society, 494(4), 5207-5229. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 494, 5207-5229
Musoke, G, Young, A J, Molnar, S M & Birkinshaw, M 2020, ' Numerical simulations of colliding jets in an external wind : application to 3C 75 ', Monthly Notices of the Royal Astronomical Society, vol. 494, no. 4, staa1071, pp. 5207-5229 . https://doi.org/10.1093/mnras/staa1071
Monthly Notices of the Royal Astronomical Society, 494(4), 5207-5229. Oxford University Press
The radio galaxy 3C 75 is remarkable because it contains a pair of radio-loud active galaxies, each of which produces a two-sided jet, with the jet beams appearing to collide and merge to the west of the galaxies. Motivated by 3C 75, we have conducte
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ffd21a7eed372f2cf3bfc52b71e5d4bd
https://doi.org/10.1093/mnras/staa1071
https://doi.org/10.1093/mnras/staa1071
Autor:
Shivaei, Irene, Popping, Gergoe, Rieke, George, Reddy, Naveen, Pope, Alexandra, Kennicutt, Robert, Mobasher, Bahram, Coil, Alison, Fudamoto, Yoshinobu, Kriek, Mariska, Lyu, Jianwei, Oesch, Pascal, Sanders, Ryan, Shapley, Alice, Siana, Brian
Publikováno v:
Shivaei, I, Popping, G, Rieke, G, Reddy, N, Pope, A, Kennicutt, R, Mobasher, B, Coil, A, Fudamoto, Y, Kriek, M, Lyu, J, Oesch, P, Sanders, R, Shapley, A & Siana, B 2022, ' Infrared Spectral Energy Distributions and Dust Masses of Sub-solar Metallicity Galaxies at z similar to 2.3 ', Astrophysical Journal, vol. 928, no. 1, 68 . https://doi.org/10.3847/1538-4357/ac54a9
We present results from Atacama Large Millimeter/submillimeter Array (ALMA) 1.2 mm continuum observations of a sample of 27 star-forming galaxies at z = 2.1-2.5 from the MOSFIRE Deep Evolution Field survey with metallicity and star formation rate mea
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2751::c7ce4b45875cbe571849b84235c1e86a
https://curis.ku.dk/portal/da/publications/infrared-spectral-energy-distributions-and-dust-masses-of-subsolar-metallicity-galaxies-at-z-similar-to-23(16a1e480-6fa0-4112-9f5c-721b8a052b62).html
https://curis.ku.dk/portal/da/publications/infrared-spectral-energy-distributions-and-dust-masses-of-subsolar-metallicity-galaxies-at-z-similar-to-23(16a1e480-6fa0-4112-9f5c-721b8a052b62).html
Autor:
J. M. Diego, A. K. Meena, N. J. Adams, T. Broadhurst, L. Dai, D. Coe, B. Frye, P. Kelly, A. M. Koekemoer, M. Pascale, S. P. Willner, E. Zackrisson, A. Zitrin, R. A. Windhorst, S. H. Cohen, R. A. Jansen, J. Summers, S. Tompkins, C. J. Conselice, S. P. Driver, H. Yan, N. Grogin, M. A. Marshall, N. Pirzkal, A. Robotham, R. E. Ryan, C. N. A. Willmer, L. D. Bradley, G. Caminha, K. Caputi, T. Carleton, P. Kamieneski
Publikováno v:
INSPIRE-HEP
The first JWST data on the massive colliding cluster El Gordo confirm 23 known families of multiply lensed images and identify 8 new members of these families. Based on these families, which have been confirmed spectroscopically by MUSE, we derived a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::17d8ae363c15bd87b17278f8aa65b6ec
https://doi.org/10.1051/0004-6361/202245238
https://doi.org/10.1051/0004-6361/202245238
Autor:
Kéruzoré, F., Mayet, F., Pratt, G. W., Adam, R., Ade, P., André, P., Andrianasolo, A., Arnaud, M., Aussel, H., Bartalucci, I., Beelen, A., Benoît, A., Berta, S., Bourrion, O., Calvo, M., Catalano, A., De Petris, M., Désert, F. -X., Doyle, S., Driessen, E. F. C., Gomez, A., Goupy, J., Kramer, C., Ladjelate, B., Lagache, G., Leclercq, S., Lestrade, J. -F., Macías-Pérez, J. F., Mauskopf, P., Monfardini, A., Perotto, L., Pisano, G., Pointecouteau, E., Ponthieu, N., Revéret, V., Ritacco, A., Romero, C., Roussel, H., Ruppin, F., Schuster, K., Shu, S., Sievers, A., Tucker, C.
Publikováno v:
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 644, pp.A93. ⟨10.1051/0004-6361/202038933⟩
Universidad de Alicante (UA)
Instituto Nacional de Técnica Aeroespacial (INTA)
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 644, pp.A93. ⟨10.1051/0004-6361/202038933⟩
Universidad de Alicante (UA)
High-resolution mapping of the intra-cluster medium (ICM) up to high redshift and down to low masses is crucial to derive accurate mass estimates of the galaxy cluster and to understand the systematic effects affecting cosmological studies based on g
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::96bdd2e0f9579515f3c2b80b2a74c5a3
https://orca.cardiff.ac.uk/id/eprint/137311/1/aa38933-20.pdf
https://orca.cardiff.ac.uk/id/eprint/137311/1/aa38933-20.pdf
Autor:
Tom Oosterloo, Raffaella Morganti, Suma Murthy, Bjorn Emonts, Reynier Peletier, M. Villar-Martín
Publikováno v:
Astronomy & astrophysics, 643:A74. EDP Sciences
Digital.CSIC. Repositorio Institucional del CSIC
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
Universidad de Alicante (UA)
Digital.CSIC. Repositorio Institucional del CSIC
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
Universidad de Alicante (UA)
The neutral atomic gas content of galaxies is usually studied in the HI 21 cm emission line of hydrogen. However, as we go to higher redshifts, owing to the weak strength of the transition, we need very deep integrations to detect HI emission. The HI
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bde9600008e4743f1b0df369185f7b39
http://arxiv.org/abs/2009.13338
http://arxiv.org/abs/2009.13338