Results 11 to 20 of about 478 (147)

A Framework for Modeling Polycyclic Aromatic Hydrocarbon Emission in Galaxy Evolution Simulations

open access: yesThe Astrophysical Journal, 2023
We present a new methodology for simulating mid-infrared emission from polycyclic aromatic hydrocarbons (PAHs) in galaxy evolution simulations. To do this, we combine theoretical models of PAH emission features as they respond to varying interstellar ...
Desika Narayanan   +9 more
doaj   +1 more source

Latest results on dark matter searches with H.E.S.S [PDF]

open access: yesEPJ Web of Conferences, 2019
The nature of Dark Matter (DM) is one of the most debated questions of contemporary physics. Ground-based arrays of Cherenkov telescopes such as the High Energy Spectroscopic System (H.E.S.S.) search for DM signatures through the detection of Very-High ...
Rinchiuso Lucia
doaj   +1 more source

Public Data Release of the FIRE-2 Cosmological Zoom-in Simulations of Galaxy Formation

open access: yesThe Astrophysical Journal Supplement Series, 2023
We describe a public data release of the FIRE-2 cosmological zoom-in simulations of galaxy formation (available at http://flathub.flatironinstitute.org/fire ) from the Feedback In Realistic Environments (FIRE) project.
Andrew Wetzel   +25 more
doaj   +1 more source

A Physical Interpretation of Milky Way Galaxy Dynamics from Precision Astrometrics

open access: yes, 2020
The dynamical and virial mass of the Milky Way galaxy is estimated using latest high precision stellar halo and dwarf galaxy satellite kinematics. The new data suggest the Galaxy is a highly compact, classically thermalized object. Kinematics exhibit significant velocity-spatial substructure, distinctive dynamic partitions, and strong Keplerian ...
openaire   +2 more sources

An innovative model of a non-relativist universe [PDF]

open access: yesE3S Web of Conferences, 2020
The paper investigates a model of the local Universe based on the concepts of nonrelativistic physics. The space-time boundaries of its applicability are estimated.
Baryshnikova Olga   +2 more
doaj   +1 more source

Connecting Star Formation in the Milky Way and Nearby Galaxies. I. Comparability of Molecular Cloud Physical Properties

open access: yesMonthly Notices of the Royal Astronomical Society
Abstract We used CO (2-1) and CO (1-0) data cubes to identify molecular clouds and study their kinematics and dynamics in three nearby galaxies and the inner Milky Way. When observed at similar spatial and velocity resolutions, molecular clouds in the same mass range across these galaxies show broadly comparable physical properties ...
J W Zhou, Sami Dib
openaire   +2 more sources

Simulating Atomic Dark Matter in Milky Way Analogs

open access: yesThe Astrophysical Journal Letters, 2023
Dark sector theories naturally lead to multicomponent scenarios for dark matter where a subcomponent can dissipate energy through self-interactions, allowing it to efficiently cool inside galaxies.
Sandip Roy   +5 more
doaj   +1 more source

Constraints on the Frequency and Mass Content of r-process Events Derived from Turbulent Mixing in Galactic Disks

open access: yesThe Astrophysical Journal, 2023
Metal-poor stars in the Milky Way (MW) halo display large star-to-star dispersion in their r -process abundance relative to lighter elements. This suggests a chemically diverse and unmixed interstellar medium (ISM) in the early universe.
Anne Noer Kolborg   +4 more
doaj   +1 more source

The Age-dependent Vertical Actions of Young Stars in the Galaxy

open access: yesThe Astrophysical Journal
Stars in the Galactic disk are born on cold, nearly circular orbits with small vertical excursions. After their birth, their orbits evolve, driven by small- or large-scale perturbations in the Galactic disk’s gravitational potential.
D. N. Garzon   +4 more
doaj   +1 more source

Spaceborne and spaceborn: Physiological aspects of pregnancy and birth during interplanetary flight

open access: yesExperimental Physiology, EarlyView.
Abstract Crewed interplanetary return missions that are on the planning horizon will take years, more than enough time for initiation and completion of a pregnancy. Pregnancy is viewed as a sequence of processes – fertilization, blastocyst formation, implantation, gastrulation, placentation, organogenesis, gross morphogenesis, birth and neonatal ...
Arun V. Holden
wiley   +1 more source

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