Zobrazeno 1 - 10
of 115
pro vyhledávání: '"ISM -ISM"'
Publikováno v:
Open Astronomy, Vol 31, Iss 1, Pp 99-105 (2022)
Extraplanar structures of ionized gas are detected in numerous edge-on galaxies. Whether HII regions or supernovae (SNe) responsible for its ionization is still debated. Here, we consider the Hα{\rm{H}}\alpha emissivity from shells of superbubbles d
Externí odkaz:
https://doaj.org/article/b3cbfaeef9c24a5c8a339f23e68032ba
Publikováno v:
Open Astronomy, Vol 26, Iss 1, Pp 224-232 (2017)
Using 3-D gas dynamic simulations, we study the supernova (SNe) driven transport of gas from the galactic disk. We assume that SNe are distributed randomly and uniformly in the galactic plane and we consider sufficiently high volume SNe rates that ar
Externí odkaz:
https://doaj.org/article/428a9c3c502e4cb79fb9c809921acef2
Publikováno v:
Open Astronomy, Vol 26, Iss 1, Pp 233-239 (2017)
It is believed that when bubbles formed by multiple supernovae explosions interact with one another, they stimulate star formation in overlapping shells. We consider the evolution of a shocked layer formed by the collision of two identical bubbles ea
Externí odkaz:
https://doaj.org/article/9e0596c9412242f999831b026f598112
Autor:
Ángeles I Díaz, S Zamora
Publikováno v:
Biblos-e Archivo. Repositorio Institucional de la UAM
Consejo Superior de Investigaciones Científicas (CSIC)
Consejo Superior de Investigaciones Científicas (CSIC)
This is a pre-copyedited, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The version of record Monthly Notices of the Royal Astronomical Society 511.3 (2022): 437
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::228a7cdb1faad460e800033ce59e26d9
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Publikováno v:
Astronomische Nachrichten. 341:184-190
A hot plasma is the dominant phase of the interstellar medium of early-type galaxies. Its origin can reside in stellar mass losses, residual gas from the formation epoch, and accretion from outside of the galaxies. Its evolution is linked to the dyna
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::92901041231b5578bfa20911b3e8a1bf
https://doi.org/10.1002/asna.202023776
https://doi.org/10.1002/asna.202023776
Autor:
J. Holdship, S. Viti
Publikováno v:
Astronomy & Astrophysics, 658:A103
Astronomy & Astrophysics
Astronomy & Astrophysics
Molecular line emission is a powerful probe of the physical conditions of astrophysical objects but can be complex to model, and it is often unclear which transitions would be the best targets for observers who wish to constrain a given parameter. We
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2a207d411e3b268bbd220dffa258d8a8
https://doi.org/10.1051/0004-6361/202142398
https://doi.org/10.1051/0004-6361/202142398
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Anton M. Koekemoer, Filippo Fraternali, Andrew Zirm, Sune Toft, K. Harrington, Michał J. Michałowski, Vernesa Smolčić, Kartik Sheth, Benjamin Magnelli, Georgios E. Magdis, E. F. Jiménez-Andrade, Johannes Staguhn, Dominik Riechers, Mark Swinbank, E. van Kampen, Peter Capak, Carlos Gómez-Guijarro, Frank Bertoldi, Emilio Romano-Diaz, G. C. Jones, Mark Sargent, Alexander Karim, F. P. Navarrete, Chris Carilli, Eva Schinnerer, Manuel Aravena
Publikováno v:
Astronomy and Astrophysics
Astronomy & astrophysics, 615(July 2018). EDP Sciences
Astronomy & astrophysics, 2018, Vol.615, pp.A25 [Peer Reviewed Journal]
Volume 615
Astronomy & Astrophysics
Astronomy & astrophysics, 615(July 2018). EDP Sciences
Astronomy & astrophysics, 2018, Vol.615, pp.A25 [Peer Reviewed Journal]
Volume 615
Astronomy & Astrophysics
We studied the molecular gas properties of AzTEC/C159, a star-forming disk galaxy at $z=4.567$. We secured $^{12}$CO molecular line detections for the $J=2\to1$ and $J=5\to4$ transitions using the Karl G. Jansky VLA and the NOEMA interferometer. The
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::76d218c7940a280929e5394127d234a2
https://hdl.handle.net/21.11116/0000-0005-CD06-E
https://hdl.handle.net/21.11116/0000-0005-CD06-E