The hestia project: simulations of the Local Group
NI Libeskind, E Carlesi, RJJ Grand… - Monthly Notices of …, 2020 - academic.oup.com
We present the hestia simulation suite: High-resolutions Environmental Simulations of The
Immediate Area, a set of cosmological simulations of the Local Group. Initial conditions …
Immediate Area, a set of cosmological simulations of the Local Group. Initial conditions …
The γ-ray emission of star-forming galaxies
M Ajello, M Di Mauro, VS Paliya… - The Astrophysical …, 2020 - iopscience.iop.org
A majority of the γ-ray emission from star-forming galaxies is generated by the interaction of
high-energy cosmic rays with the interstellar gas and radiation fields. Star-forming galaxies …
high-energy cosmic rays with the interstellar gas and radiation fields. Star-forming galaxies …
Appreciating mergers for understanding the non-linear Mbh–M*,spheroid and Mbh–M*, galaxy relations, updated herein, and the implications for the (reduced …
We present revised (black hole mass)–(spheroid stellar mass) and (black hole mass)–
(galaxy stellar mass) scaling relations based on colour-dependent (stellar mass)-to-light …
(galaxy stellar mass) scaling relations based on colour-dependent (stellar mass)-to-light …
Legacy extragalactic uv survey (legus) with the hubble space telescope. i. survey description
ABSTRACT The Legacy ExtraGalactic UV Survey (LEGUS) is a Cycle 21 Treasury program
on the Hubble Space Telescope aimed at the investigation of star formation and its relation …
on the Hubble Space Telescope aimed at the investigation of star formation and its relation …
A 12.4-day periodicity in a close binary system after a supernova
Neutron stars and stellar-mass black holes are the remnants of massive star explosions.
Most massive stars reside in close binary systems, and the interplay between the companion …
Most massive stars reside in close binary systems, and the interplay between the companion …
Galactic dark matter halos and globular cluster populations. III. Extension to extreme environments
WE Harris, JP Blakeslee, GLH Harris - The Astrophysical Journal, 2017 - iopscience.iop.org
Abstract The total mass ${M} _ {\mathrm {GCS}} $ in the globular cluster (GC) system of a
galaxy is empirically a near-constant fraction of the total mass ${M} _ {h}\equiv {M} …
galaxy is empirically a near-constant fraction of the total mass ${M} _ {h}\equiv {M} …
The Fornax Deep Survey with the VST-IV. A size and magnitude limited catalog of dwarf galaxies in the area of the Fornax cluster
Context. The Fornax Deep Survey (FDS), an imaging survey in the u′, g′, r′, and i′-
bands, has a supreme resolution and image depth compared to the previous spatially …
bands, has a supreme resolution and image depth compared to the previous spatially …
How much hydrogen is in Type Ib and IIb supernova progenitors?
Core-collapse supernovae showing little or no hydrogen (denoted by Type IIb and Ib,
respectively) are the explosions of massive stars that have lost some or most of their outer …
respectively) are the explosions of massive stars that have lost some or most of their outer …
The SAMI–Fornax Dwarfs Survey–III. Evolution of [α/Fe] in dwarfs, from Galaxy Clusters to the Local Group
J Romero-Gómez, RF Peletier… - Monthly Notices of …, 2023 - academic.oup.com
Using very deep, high spectral resolution data from the SAMI Integral Field Spectrograph,
we study the stellar population properties of a sample of dwarf galaxies in the Fornax …
we study the stellar population properties of a sample of dwarf galaxies in the Fornax …
LIGHTS. Survey Overview and a Search for Low Surface Brightness Satellite Galaxies
We present an overview of the LBT Imaging of Galactic Halos and Tidal Structures survey,
which currently includes 25 nearby galaxies that are on average∼ 1 mag fainter than the …
which currently includes 25 nearby galaxies that are on average∼ 1 mag fainter than the …