Zobrazeno 1 - 10
of 10
pro vyhledávání: '"Salome, Quentin"'
Autor:
Salomé, Quentin, Krongold, Yair, Longinotti, Anna Lia, Bischetti, Manuela, García-Burillo, Santiago, Vega, Olga, Sánchez-Portal, Miguel, Feruglio, Chiara, Jiménez-Donaire, María Jesús, Zanchettin, Maria Vittoria
We present the first systematic study of the molecular gas and star formation efficiency in a sample of ten narrow-line Seyfert 1 galaxies selected to have X-ray Ultra Fast Outflows and, therefore, to potentially show AGN feedback effects. CO observa
Externí odkaz:
http://arxiv.org/abs/2307.06087
Autor:
Longinotti, Anna Lia, Salomé, Quentin, Feruglio, Chiara, Krongold, Yair, García-Burillo, Santiago, Giroletti, Marcello, Panessa, Francesca, Stanghellini, Carlo, Vega, Olga, Patiño-Álvarez, Victor Manuel, Chavushyan, Vahram, Elías-Chavez, Mauricio, Robleto-Orús, Aitor
The Narrow Line Seyfert 1 Galaxy IRAS17020+4544 is one of the few AGN where a galaxy-scale energy-conserving outflow was revealed. This paper reports on NOEMA observations addressed to constrain the spatial scale of the CO emission in outflow. The mo
Externí odkaz:
http://arxiv.org/abs/2302.08165
Autor:
Ballesteros-Paredes, Javier, Román-Zúñiga, Carlos, Salomé, Quentin, Zamora-Avilés, Manuel, Jiménez-Donaire, María Jesús
Different studies have reported a power-law mass-size relation $M \propto R^q$ for ensembles of molecular clouds. In the case of nearby clouds, the index of the power-law $q$ is close to 2. However, for clouds spread all over the Galaxy, indexes larg
Externí odkaz:
http://arxiv.org/abs/1909.03175
Autor:
Marchal, Antoine, Miville-Deschenes, Marc-Antoine, Orieux, Francois, Gac, Nicolas, Soussen, Charles, Lesot, Marie-Jeanne, d'Allonnes, Adrien Revault, Salome, Quentin
Publikováno v:
A&A 626, A101 (2019)
Extracting the multiphase structure of the neutral interstellar medium (ISM) is key to understand the star formation in galaxies. The radiative condensation of the diffuse warm neutral medium producing a thermally unstable lukewarm medium and a dense
Externí odkaz:
http://arxiv.org/abs/1905.00658
Publikováno v:
A&A 627, A6 (2019)
NGC 5128 (Centaurus A) is one of the best targets to study AGN-feedback in the local Universe. Optical filaments located at 16 kpc from the galaxy along the radio jet direction show recent star formation, likely triggered by the interaction of the je
Externí odkaz:
http://arxiv.org/abs/1901.11148
Autor:
Salomé, Quentin, Salomé, Philippe, Miville-Deschênes, Marc-Antoine, Combes, Françoise, Hamer, Stephen
Publikováno v:
A&A 617, C3 (2018)
NGC 5128 is one of the best targets to study AGN-feedback in the local Universe. At 13.5 kpc from the galaxy, optical filaments with recent star formation lie along the radio-jet direction. It is a testbed region for positive feedback (jet-induced st
Externí odkaz:
http://arxiv.org/abs/1710.09851
NGC 5128 (Centaurus A) is one of the best example to study AGN-feedback in the local Universe. At 13.5 kpc from the galaxy, optical filaments with recent star formation are lying along the radio-jet direction. We used the Atacama Pathfinder EXperimen
Externí odkaz:
http://arxiv.org/abs/1605.05986
Publikováno v:
A&A 586, A45 (2016)
Centaurus A is the most nearby powerful AGN, widely studied at all wavelengths. Molecular gas has been found in the halo at a distance of ~20 kpc from the galaxy centre, associated with HI shells. The molecular gas lies inside some IR and UV bright s
Externí odkaz:
http://arxiv.org/abs/1511.04310
Publikováno v:
A&A 575, L3 (2015)
Evidence of AGN interaction with the IGM is observed in some galaxies and many cool core clusters. Radio jets are suspected to dig large cavities into the surrounding gas. In most cases, very large optical filaments are seen around the central galaxy
Externí odkaz:
http://arxiv.org/abs/1409.7700
Autor:
Salomé, Quentin
Les galaxies massives sont moins nombreuses que ce qui est attendu avec le modèle standard (le modèle Λ-CDM). Ceci ce traduit par une formation d’étoiles moins importante que prévue dans les galaxies. Pour expliquer celà, il est globalement a
Externí odkaz:
http://www.theses.fr/2016PSLEO005/document