Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Manuel Behrendt"'
Publikováno v:
The Astrophysical Journal Letters, Vol 971, Iss 2, p L44 (2024)
Recent hydrodynamical simulations of the late stages of supernova remnant (SNR) evolution have revealed that as they merge with the ambient medium, SNRs implode, leading to the formation of dense clouds in their center. While being highly chemically
Externí odkaz:
https://doaj.org/article/8daf1aae1174419597b6566229807656
Publikováno v:
The Astrophysical Journal, Vol 965, Iss 2, p 168 (2024)
The deposition of energy and momentum by supernova explosions has been subject to numerous studies in the past few decades. However, while there has been some work that focused on the transition from the adiabatic to the radiative stage of a supernov
Externí odkaz:
https://doaj.org/article/66dfdc4bb80c4dd0b81f30178fded153
Autor:
A. Zanella, Michael Hilker, F. Arrigoni-Battaia, Johan Richard, Francesco Valentino, Martin Zwaan, Chian-Chou Chen, Christopher Harrison, Manuel Behrendt, Eric Emsellem, Joel Vernet, Jérémy Fensch, E. Le Floc'h, Andreas Burkert, G. Rodighiero, Eros Vanzella, Pascale Hibon, Max Gronke, E. Iani, A. M. Swinbank, Vincenzo Mainieri
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 507(3), 3830-3848. Oxford University Press
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2021, 507, pp.3830-3848. ⟨10.1093/mnras/stab2376⟩
Monthly notices of the Royal Astronomical Society, 2021, Vol.507(3), pp.3830-3848 [Peer Reviewed Journal]
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2021, 507, pp.3830-3848. ⟨10.1093/mnras/stab2376⟩
Monthly notices of the Royal Astronomical Society, 2021, Vol.507(3), pp.3830-3848 [Peer Reviewed Journal]
Giant star-forming regions (clumps) are widespread features of galaxies at $z \approx 1-4$. Theory predicts that they can play a crucial role in galaxy evolution if they survive to stellar feedback for > 50 Myr. Numerical simulations show that clumps
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::51842f598cc6793076efb5ef1a45e507
https://research.rug.nl/en/publications/2dc46764-74f5-4e98-867d-932bef1c6017
https://research.rug.nl/en/publications/2dc46764-74f5-4e98-867d-932bef1c6017
Autor:
Emanuele Daddi, Baptiste Faure, Manuel Behrendt, Jérémy Fensch, Andreas Burkert, Frédéric Bournaud, Johan Richard
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2021, 502, pp.4641-4657. ⟨10.1093/mnras/stab272⟩
Monthly Notices of the Royal Astronomical Society, 2021, 502, pp.4641-4657. ⟨10.1093/mnras/stab272⟩
High-redshift star-forming galaxies have very different morphologies compared to nearby ones. Indeed, they are often dominated by bright star-forming structures of masses up to $10^{8-9}$ $\mathrm{M}_\odot$ dubbed {\guillemotleft}giant clumps{\guille
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d90fddc4eaae29da3e3cbb755dc5f761
https://hal-insu.archives-ouvertes.fr/insu-03745716
https://hal-insu.archives-ouvertes.fr/insu-03745716
Autor:
Anna Cibinel, F. Valentino, Frederic Bournaud, Masato Onodera, A. Zanella, J. Sánchez Almeida, E. Le Floc'h, Raphael Gobat, E. Bernhard, Emanuele Daddi, Andreas Burkert, Christopher Harrison, Manuel Behrendt, Jakub Scholtz, Jérémy Fensch, V. Strazzullo, M. Kohandel
Publikováno v:
Zanella, A, Le Floc'h, E, Harrison, C M, Daddi, E, Bernhard, E, Gobat, R, Strazzullo, V, Valentino, F, Cibinel, A, Sanchez Almeida, J, Kohandel, M, Fensch, J, Behrendt, M, Burkert, A, Onodera, M, Bournaud, F & Scholtz, J 2019, ' A contribution of star-forming clumps and accreting satellites to the mass assembly of z ∼ 2 galaxies ', Monthly Notices of the Royal Astronomical Society, vol. 489, no. 2, pp. 2792-2818 . https://doi.org/10.1093/mnras/stz2099
Zanella, A, Le Floc'h, E, Harrison, C M, Daddi, E, Bernhard, E, Gobat, R, Strazzullo, V, Valentino, F, Cibinel, A, Sanchez Almeida, J, Kohandel, M, Fensch, J, Behrendt, M, Burkert, A, Onodera, M, Bournaud, F & Scholtz, J 2019, ' A contribution of star-forming clumps and accreting satellites to the mass assembly of z similar to 2 galaxies ', Monthly Notices of the Royal Astronomical Society, vol. 489, no. 2, pp. 2792-2818 . https://doi.org/10.1093/mnras/stz2099
Monthly notices of the Royal Astronomical Society, 2019, Vol.489(2), pp.2792-2818 [Peer Reviewed Journal]
Zanella, A, Le Floc'h, E, Harrison, C M, Daddi, E, Bernhard, E, Gobat, R, Strazzullo, V, Valentino, F, Cibinel, A, Sanchez Almeida, J, Kohandel, M, Fensch, J, Behrendt, M, Burkert, A, Onodera, M, Bournaud, F & Scholtz, J 2019, ' A contribution of star-forming clumps and accreting satellites to the mass assembly of z similar to 2 galaxies ', Monthly Notices of the Royal Astronomical Society, vol. 489, no. 2, pp. 2792-2818 . https://doi.org/10.1093/mnras/stz2099
Monthly notices of the Royal Astronomical Society, 2019, Vol.489(2), pp.2792-2818 [Peer Reviewed Journal]
We investigate the contribution of clumps and satellites to the galaxy mass assembly. We analyzed spatially-resolved Hubble Space Telescope observations (imaging and slitless spectroscopy) of 53 star-forming galaxies at z ~ 1 - 3. We created continuu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c38629643cb60cbd58fcc187aeec033f
https://academic.oup.com/mnras/article/489/2/2792/5543959
https://academic.oup.com/mnras/article/489/2/2792/5543959
Autor:
Jeremy Mould, Manuel Behrendt, Marc Schartmann, Ric Davies, Keiichi Wada, Mark Durré, Leonard Burtscher, Andreas Burkert
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 473(1), 953-968
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society
High-resolution observations from the sub-mm to the optical wavelength regime resolve the central few 100pc region of nearby galaxies in great detail. They reveal a large diversity of features: thick gas and stellar discs, nuclear starbursts, in- and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a415e116c011f24bd04e7d82d5163310
Giant clumps are a characteristic feature of observed high-redshift disk galaxies. We propose that these kpc-sized clumps have a complex substructure and are the result of many smaller clumps self-organizing themselves into clump clusters (CC). This
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::407fdf81490efa86e36f61728a8b3223
http://arxiv.org/abs/1512.03430
http://arxiv.org/abs/1512.03430
Gravitational instabilities play an important role in structure formation of gas-rich high-redshift disc galaxies. In this paper, we revisit the axisymmetric perturbation theory and the resulting growth of structure by taking the realistic thickness
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ecb9d23862167c3197e63a4450c12eec