Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Fiorella L. Polles"'
Autor:
Fiorella L. Polles, Dario Fadda, William D. Vacca, Nicholas P. Abel, Mélanie Chevance, Christian Fischer, James M. Jackson, Vianney Lebouteiller, Suzanne Madden, Lise Ramambason
Publikováno v:
The Astronomical Journal, Vol 168, Iss 3, p 117 (2024)
We present the [O III ] λ 52 μ m map of the dwarf galaxy IC 10 obtained with the Field-Imaging Far-Infrared Line Spectrometer on board the Stratospheric Observatory for Infrared Astronomy. We combine the [O III ] λ 52 μ m map with Herschel and Sp
Externí odkaz:
https://doaj.org/article/9b56a7e9ea5645dbae44646433175c6f
Autor:
James M. Jackson, J. Scott Whitaker, Edward Chambers, Robert Simon, Cristian Guevara, David Allingham, Philippa Patterson, Nicholas Killerby-Smith, Jacob Askew, Thomas Vandenberg, Howard A. Smith, Patricio Sanhueza, Ian W. Stephens, Lars Bonne, Fiorella L. Polles, Anika Schmiedeke, Netty Honigh, Matthias Justen
Publikováno v:
The Astrophysical Journal, Vol 965, Iss 2, p 187 (2024)
Using the upGREAT instrument on board the Stratospheric Observatory for Infrared Astronomy, we imaged [C ii ] 157.74 and [O i ] 63.18 μ m line emission from a bright photodissociation region (PDR) associated with an ionized bubble located in the Nes
Externí odkaz:
https://doaj.org/article/c6acca09c3784b24a39a254e8e05e00a
Centres of galaxy clusters must be efficiently reheated to avoid a cooling catastrophe. One potential reheating mechanism is anisotropic thermal conduction, which could transport thermal energy from intermediate radii to the cluster center. However,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6fc77c0090d7951b9bb5bc71024fd2da
http://arxiv.org/abs/2204.12514
http://arxiv.org/abs/2204.12514
Autor:
Ricarda S. Beckmann, Yohan Dubois, Alisson Pellissier, Valeria Olivares, Fiorella L. Polles, Oliver Hahn, Pierre Guillard, Matthew D. Lehnert
Publikováno v:
Astronomy & Astrophysics
One of the key physical processes that helps prevent strong cooling flows in galaxy clusters is the continued energy input from the central active galactic nucleus (AGN) of the cluster. However, it remains unclear how this energy is thermalised so th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::374efc96f45ae31f23edd04a606c7667
https://hal.archives-ouvertes.fr/hal-03649424
https://hal.archives-ouvertes.fr/hal-03649424
Autor:
Sacha Hony, Dario Fadda, Remy Indebetouw, Hans Zinnecker, Elena Sabbi, Diane Cormier, Suzanne C. Madden, Fiorella L. Polles, Christof Iserlohe, Christian Fischer, Mélanie Chevance, M.-Y. Lee, William D. Vacca, Margaret Meixner, Albrecht Poglitsch, J. M. Diederik Kruijssen, Alfred Krabbe, Frédéric Galliano, Vianney Lebouteiller
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, 2020, 494 (4), pp.5279-5292. ⟨10.1093/mnras/staa1106⟩
Monthly Notices of the Royal Astronomical Society, 2020, 494 (4), pp.5279-5292. ⟨10.1093/mnras/staa1106⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 494 (4), pp.5279-5292. ⟨10.1093/mnras/staa1106⟩
Monthly Notices of the Royal Astronomical Society, 2020, 494 (4), pp.5279-5292. ⟨10.1093/mnras/staa1106⟩
Determining the efficiency with which gas is converted into stars in galaxies requires an accurate determination of the total reservoir of molecular gas mass. However, despite being the most abundant molecule in the Universe, H$_2$ is challenging to
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8deb32528ed94ab80972cdbadf98279f
https://doi.org/10.1093/mnras/staa1106
https://doi.org/10.1093/mnras/staa1106