Zobrazeno 1 - 10
of 3 331
pro vyhledávání: '"A. Rathjen"'
Autor:
Brugaletta, Vittoria, Walch, Stefanie, Naab, Thorsten, Girichidis, Philipp, Rathjen, Tim-Eric, Seifried, Daniel, Nürnberger, Pierre Colin, Wünsch, Richard, Glover, Simon C. O.
Low-metallicity environments are subject to inefficient cooling. They also have low dust-to-gas ratios and therefore less efficient photoelectric (PE) heating than in solar-neighbourhood conditions, where PE heating is one of the most important heati
Externí odkaz:
http://arxiv.org/abs/2410.19087
SILCC -- VIII: The impact of far-ultraviolet radiation on star formation and the interstellar medium
Autor:
Rathjen, Tim-Eric, Walch, Stefanie, Naab, Thorsten, Nürnberger, Pierre, Wünsch, Richard, Seifried, Daniel, Glover, Simon C. O.
We present magnetohydrodynamic simulations of star formation in the multiphase interstellar medium to quantify the impact of non-ionising far-ultraviolet (FUV) radiation. This study is carried out within the framework of the \textsc{Silcc Project}. I
Externí odkaz:
http://arxiv.org/abs/2410.00124
Autor:
Fotopoulou, Constantina M., Naab, Thorsten, Lahén, Natalia, Cernetic, Miha, Rathjen, Tim-Eric, Steinwandel, Ulrich P., Hislop, Jessica M., Walch, Stefanie, Johansson, Peter H.
We present an analysis of the cold gas phase in a low metallicity starburst generated in a high-resolution hydrodynamical simulation of a gas-rich dwarf galaxy merger as part of the GRIFFIN project. The simulations resolve (4 M$_\odot$ gas phase mass
Externí odkaz:
http://arxiv.org/abs/2408.16887
Feferman proved in 1962 that any arithmetical theorem is a consequence of a suitable transfinite iteration of full uniform reflection of $\mathsf{PA}$. This result is commonly known as Feferman's completeness theorem. The purpose of this paper is two
Externí odkaz:
http://arxiv.org/abs/2405.09275
Autor:
Simone Böbel, Ansgar Gerhardus, Carolin Herbon, Hannah Jilani, Kim Isabel Rathjen, Guido Schmiemann, Imke Schilling
Publikováno v:
Research Involvement and Engagement, Vol 10, Iss 1, Pp 1-13 (2024)
Abstract Background Patient and Public Involvement (PPI) is increasingly recognized as an essential aspect of clinical research, particularly for ensuring relevancy and impact of research to those most affected. This study addresses the gap in involv
Externí odkaz:
https://doaj.org/article/66edb16995a047fc8aac9d58dd27da9f
Autor:
Makarenko, Ekaterina I., Walch, Stefanie, Clarke, Seamus D., Seifried, Daniel, Naab, Thorsten, Nürnberger, Pierre C., Rathjen, Tim-Eric
Supernovae (SNe) inject $\sim 10^{51}$ erg in the interstellar medium, thereby shocking and heating the gas. A substantial fraction of this energy is later lost via radiative cooling. We present a post-processing module for the FLASH code to calculat
Externí odkaz:
http://arxiv.org/abs/2305.07652
Autor:
Shu, Shuangshuang, Rathjen, Michael
We prove that, over Kripke-Platek set theory with infinity (KP), transfinite induction along the ordinal ${\epsilon}_{\Omega+1}$ is equivalent to the schema asserting the soundness of KP, where $\Omega$ denotes the supremum of all ordinals in the uni
Externí odkaz:
http://arxiv.org/abs/2212.02843
Autor:
Rathjen, Tim-Eric, Naab, Thorsten, Walch, Stefanie, Seifried, Daniel, Girichidis, Philipp, Wünsch, Richard
We present magnetohydrodynamic (MHD) simulations of the star-forming multiphase interstellar medium (ISM) in stratified galactic patches with gas surface densities $\Sigma_\mathrm{gas} =$ 10, 30, 50, and 100 $\mathrm{M_\odot\,pc^{-2}}$. The SILCC pro
Externí odkaz:
http://arxiv.org/abs/2211.15419
Autor:
Matthews, Richard, Rathjen, Michael
We study the properties of the constructible universe, L, over intuitionistic theories. We give an extended set of fundamental operations which is sufficient to generate the universe over Intuitionistic Kripke-Platek set theory without Infinity. Foll
Externí odkaz:
http://arxiv.org/abs/2206.08283
We analyse synthetic $^{12}$CO, $^{13}$CO, and [CII] emission maps of simulated molecular clouds of the SILCC-Zoom project, which include an on-the-fly evolution of H$_2$, CO, and C$^+$. We use simulations of hydrodynamical and magnetohydrodynamical
Externí odkaz:
http://arxiv.org/abs/2206.06393