Zobrazeno 1 - 10
of 48
pro vyhledávání: '"Chantal Balkowski"'
Autor:
A. Boselli, L. Chemin, Oscar F. Hernández, Chantal Balkowski, M.-M. de Denus-Baillargeon, Philippe Amram, Claude Carignan, Isabelle Dicaire, Kambiz Fathi, Olivier Daigle, Robert C. Kennicutt
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2008, 385, pp.553-605. ⟨10.1111/j.1365-2966.2008.12868.x⟩
Monthly Notices of the Royal Astronomical Society, 2008, 385, pp.553-605. ⟨10.1111/j.1365-2966.2008.12868.x⟩
International audience; This is the second part of an Halpha kinematics follow-up survey of the Spitzer Infrared Nearby Galaxies Survey (SINGS) sample. The aim of this paper is to shed new light on the role of baryons and their kinematics and on the
Autor:
Joel Vernet, Nicole P. H. Nesvadba, C. J. Cesarsky, Herve Wozniak, Hector Flores, S. diSeregoAlighieri, I. Fuentes-Carrera, D. Vergani, M. D. Lehnert, B. Guiderdoni, Lucia Pozzetti, Ajit K. Kembhavi, Benoit Neichel, Mathieu Puech, F. Hammer, Yun-Feng Liang, Helmut Dannerbauer, Göran Östlin, P. Amram, Chantal Balkowski, C. D. Ravikumar, Y. Yang, A. Rawat
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2008, 477, pp.789-805. ⟨10.1051/0004-6361:20078219⟩
Astronomy and Astrophysics-A&A, 2008, 477, pp.789-805. ⟨10.1051/0004-6361:20078219⟩
(abbreviated) We present the first results of the ESO large program, ``IMAGES'' which aims at obtaining robust measurements of the kinematics of distant galaxies using the multi-IFU mode of GIRAFFE on the VLT. 3D spectroscopy is essential to robustly
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2007, 471, pp.753-764. ⟨10.1051/0004-6361:20054069⟩
Astronomy and Astrophysics-A&A, 2007, 471, pp.753-764. ⟨10.1051/0004-6361:20054069⟩
International audience; Context: HCG 31 is one of the most intriguing compact groups in Hickson's catalogue. It contains a central pair of interacting dwarf galaxies and other small members that are highly peculiar. Aims: The main goal of this study
Autor:
Ana Laura Serra, Emilio J. Alfaro, Ismael Perez-Fournon, J. M. Rodríguez-Espinosa, S. Temporin, Andrea Biviano, Jordi Cepa, B. McBreen, Irene Pintos-Castro, C. P. Haines, Bianca M. Poggianti, Alfonso Aragón-Salamanca, N. Castro-Rodriguez, Ivan Oteo, Ricardo Pérez-Martínez, M. Ramón-Pérez, Francisco J. Castander, Ian Smail, Chantal Balkowski, Pierre-Alain Duc, Helena Domínguez-Sánchez, I. Gonzalez-Serrano, Antonaldo Diaferio, Malcom Bremer, J. S. Santos, D. Coia, Ángel Bongiovanni, Miguel Sánchez-Portal, Ana L. Chies-Santos, Ivan Valtchanov, J. Polednikova, Graham P. Smith, Bruno Altieri, Alessandro Ederoclite, Héctor O. Castañeda, James E. Geach, Ana María Pérez García, L. Metcalfe
Publikováno v:
Astronomy & astrophysics, 2015, Vol.578, pp.A30 [Peer Reviewed Journal]
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2015, 578, pp.A30. ⟨10.1051/0004-6361/201525620⟩
Astronomy and Astrophysics-A&A, 2015, 578, pp.A30. ⟨10.1051/0004-6361/201525620⟩
ResearcherID
Sánchez-Portal, M, Pintos-Castro, I, Pérez-Martínez, R, Cepa, J, Pérez García, A M, Domínguez-Sánchez, H, Bongiovanni, A, Serra, A L, Alfaro, E, Altieri, B, Aragón-Salamanca, A, Balkowski, C, Biviano, A, Bremer, M, Castander, F, Castañeda, H, Castro-Rodríguez, N, Chies-Santos, A L, Coia, D, Diaferio, A, Duc, P A, Ederoclite, A, Geach, J, González-Serrano, I, Haines, C P, McBreen, B, Metcalfe, L, Oteo, I, Pérez-Fournón, I, Poggianti, B, Polednikova, J, Ramón-Pérez, M, Rodríguez-Espinosa, J M, Santos, J S, Smail, I, Smith, G P, Temporin, S & Valtchanov, I 2015, ' GLACE survey : OSIRIS/GTC tuneable filter Hα imaging of the rich galaxy cluster ZwCl 0024.0+1652 at z = 0.395. I. Survey presentation, TF data reduction techniques, and catalogue ', Astronomy and Astrophysics, vol. 578, A30 . https://doi.org/10.1051/0004-6361/201525620
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2015, 578, pp.A30. ⟨10.1051/0004-6361/201525620⟩
Astronomy and Astrophysics-A&A, 2015, 578, pp.A30. ⟨10.1051/0004-6361/201525620⟩
ResearcherID
Sánchez-Portal, M, Pintos-Castro, I, Pérez-Martínez, R, Cepa, J, Pérez García, A M, Domínguez-Sánchez, H, Bongiovanni, A, Serra, A L, Alfaro, E, Altieri, B, Aragón-Salamanca, A, Balkowski, C, Biviano, A, Bremer, M, Castander, F, Castañeda, H, Castro-Rodríguez, N, Chies-Santos, A L, Coia, D, Diaferio, A, Duc, P A, Ederoclite, A, Geach, J, González-Serrano, I, Haines, C P, McBreen, B, Metcalfe, L, Oteo, I, Pérez-Fournón, I, Poggianti, B, Polednikova, J, Ramón-Pérez, M, Rodríguez-Espinosa, J M, Santos, J S, Smail, I, Smith, G P, Temporin, S & Valtchanov, I 2015, ' GLACE survey : OSIRIS/GTC tuneable filter Hα imaging of the rich galaxy cluster ZwCl 0024.0+1652 at z = 0.395. I. Survey presentation, TF data reduction techniques, and catalogue ', Astronomy and Astrophysics, vol. 578, A30 . https://doi.org/10.1051/0004-6361/201525620
The cores of clusters at 0 $\lesssim$ z $\lesssim$ 1 are dominated by quiescent early-type galaxies, whereas the field is dominated by star-forming late-type ones. Galaxy properties, notably the star formation (SF) ability, are altered as they fall i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1707ab7391c5fcdd640fbfdbadacacf4
http://hdl.handle.net/2318/1522035
http://hdl.handle.net/2318/1522035
Publikováno v:
The Astrophysical Journal. 605:L17-L20
We have discovered four intergalactic H II regions in Stephan's quintet, which is more than a 25 kpc projected distance from the center of the nearest group galaxy, with no apparent optical connection to it. They have MB ranging from -11.9 to -12.5 m
Publikováno v:
The Astronomical Journal
The Astronomical Journal, 2003, 126, pp.2635-2643. ⟨10.1086/379295⟩
The Astronomical Journal, 2003, 126, pp.2635-2643. ⟨10.1086/379295⟩
We investigate the properties of the B-band Tully-Fisher (T-F) relation for 25 compact group galaxies, using Vmax derived from 2-D velocity maps. Our main result is that the majority of the Hickson Compact Group galaxies lie on the T-F relation. Howe
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2003, 402, pp.865-877. ⟨10.1051/0004-6361:20030034⟩
Astronomy and Astrophysics-A&A, 2003, 402, pp.865-877. ⟨10.1051/0004-6361:20030034⟩
International audience; We present Fabry Perot observations of galaxies in five Hickson Compact Groups: HCG 10, HCG 19, HCG 87, HCG 91 and HCG 96. We observed a total of 15 galaxies and we have detected ionized gas for 13 of them. We were able to der
Publikováno v:
Astrophysics and Space Science. 284:917-920
A description is given of the samples of Low Surface Brightness galaxies (LSBs) used for comparison with models of their chemical and spectro-photometric evolution (Boissier et al., this Volume). These samples show the large variation and scatter in
Autor:
S. Torres-Flores, Henri Plana, M. Marcelin, D. Olave-Rojas, P. Amram, C. Mendes de Oliveira, Chantal Balkowski
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2014, 442 (3), pp.2188--2201. ⟨10.1093/mnras/stu1002⟩
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Monthly Notices of the Royal Astronomical Society, 2014, 442 (3), pp.2188--2201. ⟨10.1093/mnras/stu1002⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2014, 442 (3), pp.2188--2201. ⟨10.1093/mnras/stu1002⟩
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Monthly Notices of the Royal Astronomical Society, 2014, 442 (3), pp.2188--2201. ⟨10.1093/mnras/stu1002⟩
We present new Fabry-Perot observations for a sample of 42 galaxies located in twelve compact groups of galaxies: HCG 1, HCG 14, HCG 25, HCG 44, HCG 53, HCG 57, HCG 61, HCG 69, HCG 93, VV 304, LGG 455 and Arp 314. From the 42 observed galaxies, a tot
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f4ba386a4023f415d49631fb5aac0ead
http://arxiv.org/abs/1406.0828
http://arxiv.org/abs/1406.0828
Publikováno v:
Astrophysics and Space Science. 276:459-465
We present new HI and CO data including velocity information of NGC 4548, an anaemic galaxy in the Virgo Cluster. The distribution of the atomic gas shows a ring-like structure. The HI rotation curve is deduced and can be extrapolated inwards with th