Zobrazeno 1 - 10
of 8 869
pro vyhledávání: '"dynamical equilibrium"'
Autor:
Ellison, Sara L., Pan, Hsi-An, Bluck, Asa F. L., Krumholz, Mark R., Lin, Lihwai, Hunt, Leslie, Corbelli, Edvige, Thorp, Mallory D., Barrera-Ballesteros, Jorge, Sanchez, Sebastian F., Scudder, Jillian M., Quai, Salvatore
We present the extended ALMA MaNGA QUEnching and STar formation survey, a combination of the original 46 ALMaQUEST galaxies plus new ALMA observations for a further 20 interacting galaxies. Three well-studied scaling relations are fit to the 19,999 s
Externí odkaz:
http://arxiv.org/abs/2312.03132
Autor:
Tonti, Luca1 (AUTHOR), García Daza, Fabián A.2 (AUTHOR), Romero-Enrique, José Manuel3,4 (AUTHOR), Patti, Alessandro1,4,5 (AUTHOR) apatti@ugr.es
Publikováno v:
Journal of Chemical Physics. 3/28/2024, Vol. 160 Issue 12, p1-12. 12p.
Autor:
Pieczarka, Maciej, Bleu, Olivier, Estrecho, Eliezer, Wurdack, Matthias, Steger, Mark, Snoke, David W., West, Kenneth, Pfeiffer, Loren N., Truscott, Andrew G., Ostrovskaya, Elena A., Levinsen, Jesper, Parish, Meera M.
The classic Bogoliubov theory of weakly interacting Bose gases rests upon the assumption that nearly all the bosons condense into the lowest quantum state at sufficiently low temperatures. Here we develop a generalized version of Bogoliubov theory fo
Externí odkaz:
http://arxiv.org/abs/2112.03768
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Autor:
Hewitt, C. G.
The Einstein field equations for a class of irrotational non-orthogonally transitive $G_{2}$ cosmologies are written down as a system of partial differential equations. The equilibrium points are self-similar and can be written as a one-parameter, fi
Externí odkaz:
http://arxiv.org/abs/2103.16431
We consider a class of inhomogeneous self-similar cosmological models in which the perfect fluid flow is tangential to the orbits of a three-parameter similarity group. We restrict the similarity group to possess both an Abelian $G_{2}$, and a single
Externí odkaz:
http://arxiv.org/abs/2103.16428
Autor:
Zhuravlev, V. M.1,2 (AUTHOR) zhvictorm@gmail.com
Publikováno v:
Journal of Experimental & Theoretical Physics. Dec2022, Vol. 135 Issue 6, p813-841. 29p.
Autor:
Jin, Mengting1,2 (AUTHOR), Ravi, Manoj3,4 (AUTHOR), Lei, Chen1 (AUTHOR), Heard, Christopher J.1 (AUTHOR), Brivio, Federico1,5 (AUTHOR), Tošner, Zdeněk1 (AUTHOR), Grajciar, Lukáš1 (AUTHOR) lukas.grajciar@natur.cuni.cz, van Bokhoven, Jeroen A.3,6 (AUTHOR) Jeroen.vanbokhoven@chem.ethz.ch, Nachtigall, Petr1 (AUTHOR)
Publikováno v:
Angewandte Chemie. Aug2023, Vol. 135 Issue 31, p1-6. 6p.
The dynamical stability of massive thin shells with a given equation of state (EOS) is here compared (both for the barotropic and non-barotropic case) with the results coming from thermodynamical stability. Our results show that the restrictions in t
Externí odkaz:
http://arxiv.org/abs/2006.06766
Autor:
Sun, Jiayi, Leroy, Adam K., Ostriker, Eve C., Hughes, Annie, Rosolowsky, Erik, Schruba, Andreas, Schinnerer, Eva, Blanc, Guillermo A., Faesi, Christopher, Kruijssen, J. M. Diederik, Meidt, Sharon, Utomo, Dyas, Bigiel, Frank, Bolatto, Alberto D., Chevance, Mélanie, Chiang, I-Da, Dale, Daniel, Emsellem, Eric, Glover, Simon C. O., Grasha, Kathryn, Henshaw, Jonathan, Herrera, Cinthya N., Jimenez-Donaire, Maria Jesus, Lee, Janice C., Pety, Jérôme, Querejeta, Miguel, Saito, Toshiki, Sandstrom, Karin, Usero, Antonio
Publikováno v:
ApJ, 892, 148 (2020)
We compare the observed turbulent pressure in molecular gas, $P_\mathrm{turb}$, to the required pressure for the interstellar gas to stay in equilibrium in the gravitational potential of a galaxy, $P_\mathrm{DE}$. To do this, we combine arcsecond res
Externí odkaz:
http://arxiv.org/abs/2002.08964