Zobrazeno 1 - 10
of 1 071
pro vyhledávání: '"Intergalactic star"'
Autor:
Puertas, S. Duarte, Vilchez, J. M., Iglesias-Páramo, J., Drissen, L., Kehrig, C., Martin, T., Pérez-Montero, E., Arroyo-Polonio, A.
Publikováno v:
A&A 645, A57 (2021)
Based on SITELLE spectroscopy, we studied the ionised gas emission for the 175 H$\alpha$ emission regions in the Stephan's Quintet (SQ). A detailed analysis is performed of the star formation rate (SFR), oxygen abundance (O/H), and nitrogen-to-oxygen
Externí odkaz:
http://arxiv.org/abs/2011.09924
Publikováno v:
A&A 629, A102 (2019)
Stephan's Quintet (SQ), the prototypical compact group of galaxies in the local Universe, has been observed with the imaging Fourier transform spectrometer SITELLE, attached to the CFHT, to perform a deep search for intergalactic star-forming emissio
Externí odkaz:
http://arxiv.org/abs/1909.05797
A spectroscopic analysis of 10 intergalactic star forming objects (ISFOs) and a photometric analysis of 67 ISFOs in a sample of 14 interacting systems is presented. The majority of the ISFOs have relative polycyclic aromatic hydrocarbon (PAH) band st
Externí odkaz:
http://arxiv.org/abs/1405.1274
Autor:
Duc, Pierre-Alain, Boquien, Meederic, Braine, Jonathan, Brinks, Elias, Lisenfeld, Ute, Charmandaris, Vassilis
Star formation in interacting systems may take place in various locations, from the dust--enshrouded core of Ultraluminous Infrared Galaxies to more unusual places such as the debris of colliding galaxies expelled into the intergalactic medium. Deter
Externí odkaz:
http://arxiv.org/abs/astro-ph/0610392
Star formation (SF) takes place in unusual places such as way out in the intergalactic medium out of material expelled from parent galaxies. We wish to answer whether SF proceeds in this specific environment in a similar way than in galactic disks. W
Externí odkaz:
http://arxiv.org/abs/astro-ph/0703002
Publikováno v:
NewAstron.Rev.51:63-66,2007
We present $^{12}$CO(1-0) observations of the interacting galaxy system Arp 94, which contains the Seyfert galaxies NGC 3227 and NGC 3226 as well as the star-forming candidate dwarf galaxy J1023+1952. We mapped the CO distribution in J1023+1952 with
Externí odkaz:
http://arxiv.org/abs/astro-ph/0610080
Akademický článek
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Akademický článek
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Autor:
J. Iglesias-Páramo, A. Arroyo-Polonio, Thomas Martin, Enrique Pérez-Montero, S. Duarte Puertas, C. Kehrig, Laurent Drissen, José M. Vílchez
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
Based on SITELLE spectroscopy data, we studied the ionised gas emission for the 175 H alpha emission regions in the Stephan's Quintet (SQ). In this paper we perform a detailed analysis of the star formation rate (SFR), oxygen abundance, and nitrogen-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e602b1906648d04908b9fd0b831dfa14
http://hdl.handle.net/10261/238662
http://hdl.handle.net/10261/238662
Autor:
Laurent Drissen, José M. Vílchez, C. Kehrig, Thomas P. Martin, S. Duarte Puertas, J. Iglesias-Páramo
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
Stephan's Quintet (SQ), the prototypical compact group of galaxies in the local Universe, has been observed with the imaging Fourier transform spectrometer SITELLE, attached to the Canada-France-Hawaii-Telescope, to perform a deep search for intergal
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6c3f2dff5fd70223d335509e8aa80281
http://hdl.handle.net/10261/191932
http://hdl.handle.net/10261/191932