Zobrazeno 1 - 10
of 179
pro vyhledávání: '"S. C. Madden"'
Autor:
L. Ramambason, V. Lebouteiller, A. Bik, C. T. Richardson, F. Galliano, D. Schaerer, C. Morisset, F. L. Polles, S. C. Madden, M. Chevance, I. De Looze
Publikováno v:
ASTRONOMY & ASTROPHYSICS
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, ⟨10.1051/0004-6361/202243866⟩
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, ⟨10.1051/0004-6361/202243866⟩
(abridged) Quantifying the ISM porosity to ionizing photons in nearby galaxies may improve our understanding of the mechanisms leading to Lyman Continuum photons leakage from galaxies. Primitive galaxies with low metal and dust content have been show
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c821b6e5c02565036d1b061569b0f082
http://arxiv.org/abs/2207.06146
http://arxiv.org/abs/2207.06146
Autor:
A. Beck, V. Lebouteiller, S. C. Madden, C. Iserlohe, A. Krabbe, L. Ramambason, C. Fischer, M. Kaźmierczak-Barthel, S. T. Latzko, J. P. Pérez-Beaupuits
Context. Massive star-formation leads to enrichment with heavy elements of the interstellar medium. On the other hand, the abundance of heavy elements is a key parameter to study the star-formation history of galaxies. Furthermore, the total molecula
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8a6f4f701a452cbc6d63afa405bd00f9
http://arxiv.org/abs/2206.15062
http://arxiv.org/abs/2206.15062
Autor:
S. Bianchi, M. Murgia, A. Melis, V. Casasola, F. Galliano, F. Govoni, A. P. Jones, S. C. Madden, R. Paladino, F. Salvestrini, E. M. Xilouris, N. Ysard
We observed four nearby spiral galaxies (NGC 3627, NGC 4254, NGC 4736 and NGC 5055) in the K band with the 64-m Sardinia Radio Telescope, with the aim of detecting the Anomalous Microwave Emission (AME), a radiation component presumably due to spinni
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d31f98e8cfd41ffb56ae1c1f2d404568
http://arxiv.org/abs/2201.09615
http://arxiv.org/abs/2201.09615
Autor:
A. Lambert-Huyghe, S. C. Madden, V. Lebouteiller, F. Galliano, N. Abel, D. Hu, L. Ramambason, F. L. Polles
Publikováno v:
Astronomy & Astrophysics. 666:A112
Context. The [O iii]λ88 µm line is observed in many galaxies including our neighboring Magellanic Clouds and is a well-known tracer of H ii regions, while the 24 µm continuum emission has often been used to trace warm dust in the ionized phases of
Autor:
C J R Clark, P De Vis, M Baes, S Bianchi, V Casasola, L P Cassarà, J I Davies, W Dobbels, S Lianou, I De Looze, R Evans, M Galametz, F Galliano, A P Jones, S C Madden, A V Mosenkov, S Verstocken, S Viaene, E M Xilouris, N Ysard
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 514:621-621
Autor:
Helmut Dannerbauer, Georgios E. Magdis, Annagrazia Puglisi, Jeyhan S. Kartaltepe, Isabella Cortzen, M.-Y. Lee, Daizhong Liu, Yang Gao, E. Le Floc'h, Frédéric Bournaud, Manuel Aravena, C. Gómez-Guijarro, Shuowen Jin, Raphael Gobat, Mark Dickinson, Vasily Kokorev, S. C. Madden, Emanuele Daddi, Francesco Valentino, D. B. Sanders
Publikováno v:
Astronomy & astrophysics, 2020, Vol.641, pp.A155 [Peer Reviewed Journal]
Valentino, F, Daddi, E, Puglisi, A, Magdis, G E, Liu, D, Kokorev, V, Cortzen, I, Madden, S, Aravena, M, Gómez-Guijarro, C, Lee, M-Y, Le Floc'h, E, Gao, Y, Gobat, R, Bournaud, F, Dannerbauer, H, Jin, S, Dickinson, M E, Kartaltepe, J & Sanders, D 2020, ' CO emission in distant galaxies on and above the main sequence ', Astronomy & Astrophysics, vol. 641, A155 . https://doi.org/10.1051/0004-6361/202038322
Astronomy & Astrophysics
Valentino, F, Daddi, E, Puglisi, A, Magdis, G E, Liu, D, Kokorev, V, Cortzen, I, Madden, S, Aravena, M, Gómez-Guijarro, C, Lee, M-Y, Le Floc'h, E, Gao, Y, Gobat, R, Bournaud, F, Dannerbauer, H, Jin, S, Dickinson, M E, Kartaltepe, J & Sanders, D 2020, ' CO emission in distant galaxies on and above the main sequence ', Astronomy & Astrophysics, vol. 641, A155 . https://doi.org/10.1051/0004-6361/202038322
Astronomy & Astrophysics
We present the detection of multiple CO line transitions with ALMA in a few tens of infrared-selected galaxies on and above the main sequence at z=1.1-1.7. We reliably detected the emission of CO(5-4), CO(2-1), and CO(7-6)+[CI](2-1) in 50, 33, and 13
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::669d815bb3030e788edda9b8ad024f37
Publikováno v:
Astronomy & Astrophysics
Autor:
I. De Looze, Jonathan Ivor Davies, A. Nersesian, Letizia P. Cassarà, Maud Galametz, Maarten Baes, Viviana Casasola, Edvige Corbelli, S. Viaene, S. C. Madden, P. De Vis, Anthony P. Jones, Laura Magrini, Christopher J. R. Clark, Emmanuel M. Xilouris, Jacopo Fritz, Ana Trčka, Frédéric Galliano, Aleksandr V. Mosenkov, Simone Bianchi, W. Dobbels
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 633, pp.A100. ⟨10.1051/0004-6361/201936665⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 633, pp.A100. ⟨10.1051/0004-6361/201936665⟩
ASTRONOMY & ASTROPHYSICS
Astronomy and Astrophysics-A&A, 2020, 633, pp.A100. ⟨10.1051/0004-6361/201936665⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 633, pp.A100. ⟨10.1051/0004-6361/201936665⟩
ASTRONOMY & ASTROPHYSICS
The purpose of this work is the characterization of the main scaling relations between all the ISM components (dust, atomic/molecular/total gas), gas-phase metallicity, and other galaxy properties, such as Mstar and galaxy morphology, for late-type g
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e85954979c072b89e2c1a124089131a2
https://cea.hal.science/cea-02446528/document
https://cea.hal.science/cea-02446528/document
Autor:
Emmanuel M. Xilouris, Anthony P. Jones, Nathalie Ysard, A. Nersesian, Frédéric Galliano, Christopher J. R. Clark, Simone Bianchi, Ana Trčka, I. De Looze, Maud Galametz, Viviana Casasola, Sébastien Viaene, John K. Davies, S. C. Madden, Jacopo Fritz, Aleksandr V. Mosenkov, Wouter Dobbels, S. Verstocken, Letizia P. Cassarà, Maarten Baes, P. De Vis
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 638, pp.A150. ⟨10.1051/0004-6361/202037476⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 638, pp.A150. ⟨10.1051/0004-6361/202037476⟩
ASTRONOMY & ASTROPHYSICS
Astronomy and Astrophysics-A&A, 2020, 638, pp.A150. ⟨10.1051/0004-6361/202037476⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 638, pp.A150. ⟨10.1051/0004-6361/202037476⟩
ASTRONOMY & ASTROPHYSICS
Dust emission, an important diagnostic of star formation and ISM mass throughout the Universe, can be powered by sources unrelated to ongoing star formation. In the framework of the DustPedia project we have set out to disentangle the radiation of th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a94d5a0f756debdf5fddb2078e3bb35b
Autor:
S. C. Madden, Andrew J. Levan, V. Arumugam, E. Le Floc'h, Frederic Bournaud, S. Roychowdhury, D. Cormier, Martin Zwaan, Florent Renaud, Lise Christensen, Elena Pian, M. Arabsalmani
Publikováno v:
The Astrophysical Journal
Astrophys.J.
Astrophys.J., 2020, 899 (2), pp.165. ⟨10.3847/1538-4357/aba3c0⟩
Arabsalmani, M, Renaud, F, Roychowdhury, S, Arumugam, V, Floc'h, E L, Bournaud, F, Cormier, D, Zwaan, M A, Christensen, L, Pian, E, Madden, S & Levan, A 2020, ' Local Starburst Conditions and Formation of GRB 980425/SN 1998bw within a Collisional Ring ', Astrophysical Journal, vol. 899, no. 2, 165 . https://doi.org/10.3847/1538-4357/aba3c0
Astrophys.J.
Astrophys.J., 2020, 899 (2), pp.165. ⟨10.3847/1538-4357/aba3c0⟩
Arabsalmani, M, Renaud, F, Roychowdhury, S, Arumugam, V, Floc'h, E L, Bournaud, F, Cormier, D, Zwaan, M A, Christensen, L, Pian, E, Madden, S & Levan, A 2020, ' Local Starburst Conditions and Formation of GRB 980425/SN 1998bw within a Collisional Ring ', Astrophysical Journal, vol. 899, no. 2, 165 . https://doi.org/10.3847/1538-4357/aba3c0
We present the first spatially resolved study of molecular gas in the vicinity of a Gamma Ray Burst, using CO(2-1) emission line observations with the Atacama Large Millimetre Array (ALMA) at ~50 pc scales. The host galaxy of GRB 980425 contains a ri