We also find that both entropy production after shock formation and the acceleration of the wind due to stresses produced by the waves prior to shock formation impact the structure and nucleosynthesis of these waves.
High Energy Astrophysical Phenomena Solar and Stellar Astrophysics
The combination of $f\sigma_8$ and Planck measurements prefers an even higher growth index of $\gamma=0. 639^{+0. 024}_{-0. 025}$, corresponding to a 4. 2$\sigma$-tension with the concordance model.
Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology
Furthermore, dust composition comprising amorphous carbon is found to be favorable to simultaneously account for the faint scattered light and the flared disk morphology.
Earth and Planetary Astrophysics
We implement a multi-component Gaussian fitting on the molecular data to study the kinematics.
Astrophysics of Galaxies
However, existing approaches have neglected the fact that, apart from the data labelled by amateurs, (limited) expert knowledge of the problem is also available along with vast amounts of unlabelled data that have not yet been exploited within a unified learning framework.
Astrophysics of Galaxies Instrumentation and Methods for Astrophysics Image and Video Processing
The STIX Data Center is operated at the University of Applied Sciences and Arts Northwestern Switzerland (FHNW) and consists of automated processing pipelines and a data platform.
Solar and Stellar Astrophysics Instrumentation and Methods for Astrophysics
The black hole populations in Astrid include black holes down to 10$^{4. 5}$ M$_\odot$, and remain broadly consistent with the TNG simulations at scales > 10$^6$ M$_\odot$ (the seed mass used in TNG).
Astrophysics of Galaxies
We develop a novel statistical approach to identify emission features or set upper limits in high-resolution spectra in the presence of high background.
Instrumentation and Methods for Astrophysics High Energy Astrophysical Phenomena Data Analysis, Statistics and Probability Applications
Fast radio bursts (FRBs) are being detected with increasing regularity.
Instrumentation and Methods for Astrophysics High Energy Astrophysical Phenomena
In this paper, we extend the application of MFs to CMB polarisation data by introducing a new formalism, where we lift the spin $2$ polarisation field to a scalar function in a higher dimensional manifold: the group of rotations of the sphere, $SO(3)$.
Cosmology and Nongalactic Astrophysics
