Moreover, we find that massive NSs $ > 2\, M_{\odot}$ are expected to be commonly detected in BHNS mergers in almost all our model variations.
HIGH ENERGY ASTROPHYSICAL PHENOMENA
The massive neutrinos of the Cosmic Neutrino Background (C$\nu$B) are fundamental ingredients of the radiation-dominated early universe and are important non-relativistic probes of the large-scale structure formation in the late universe.
COSMOLOGY AND NONGALACTIC ASTROPHYSICS INSTRUMENTATION AND METHODS FOR ASTROPHYSICS
The uncertainties in the evaluation of the spectra of these secondary cosmic rays, due to spallation cross sections, have been taken into account introducing a scale factor as a nuisance parameter in the fits, assuming that this uncertainty is mostly due to the normalization of the cross sections parametrizations.
HIGH ENERGY ASTROPHYSICAL PHENOMENA
In addition to tracing the standard galaxy properties, Dusty SAGE also tracks cold dust mass in the interstellar medium (ISM), hot dust mass in the halo and dust mass ejected by feedback activity.
ASTROPHYSICS OF GALAXIES
To better understand the influence of the B orbit on the TWA 3A circumbinary disk, we performed SPH simulations of the system and found that the outer edge of the gas disk ($r_\mathrm{outer}=8. 5\pm0. 2$ au) is most consistent with truncation from a coplanar, circular or moderately eccentric orbit, supporting the preference from the joint orbital fit.
We present a 5A-100um Spectral Energy Distribution (SED) of the ultracool dwarf star TRAPPIST-1, obtained as part of the Mega-MUSCLES Treasury Survey.
SOLAR AND STELLAR ASTROPHYSICS
For dwarfs of $3500<T_{eff}<5280$ K, we use metallicity values of 4, 378 stars from APOGEE and Hejazi et al. (2020) to calibrate the relationship, producing results with a $1\sigma$ precision of 0. 12 dex and few systematic errors.
SOLAR AND STELLAR ASTROPHYSICS ASTROPHYSICS OF GALAXIES INSTRUMENTATION AND METHODS FOR ASTROPHYSICS
The evolution of a single raindrop falling below a cloud is governed by fluid dynamics and thermodynamics fundamentally transferable to planetary atmospheres beyond modern Earth's.
EARTH AND PLANETARY ASTROPHYSICS ATMOSPHERIC AND OCEANIC PHYSICS
The total reconstructed velocity field at the position of the LG, smoothed with a $1 \; h^{-1} \, \mathrm{Mpc}$ Gaussian, is $552 \pm 71 \; \mathrm{km} \, \mathrm{s}^{-1}$ towards $l = 274. 3 \pm 7. 9^\circ$, $b = 33. 9 \pm 8. 1^\circ$, in good agreement with the observed CMB dipole.
COSMOLOGY AND NONGALACTIC ASTROPHYSICS
We also show that SegU-Net can be used to recover various topological summary statistics, such as size distributions and Betti numbers, with a relative difference of only a few per cent.
INSTRUMENTATION AND METHODS FOR ASTROPHYSICS