The ALMA REBELS Survey: dust continuum detections at z > 6.5
H Inami, HSB Algera, S Schouws… - Monthly Notices of …, 2022 - academic.oup.com
We report 18 dust continuum detections (≥ 3.3 σ) at∼ 88 and 158 out of 49 ultraviolet (UV)-
bright galaxies (M UV<− 21.3 mag) at> 6.5, observed by the Cycle-7 Atacama Large …
bright galaxies (M UV<− 21.3 mag) at> 6.5, observed by the Cycle-7 Atacama Large …
The ALMA REBELS Survey. Epoch of Reionization giants: Properties of dusty galaxies at z ≈ 7
We analyse FIR dust continuum measurements for 14 galaxies (redshift z≈ 7) in the ALMA
Reionization Era Bright Emission Line Survey (REBELS) Large Program to derive their …
Reionization Era Bright Emission Line Survey (REBELS) Large Program to derive their …
Tracing the primordial chemical life of glycine: a review from quantum chemical simulations
Glycine (Gly), NH2CH2COOH, is the simplest amino acid. Although it has not been directly
detected in the interstellar gas-phase medium, it has been identified in comets and …
detected in the interstellar gas-phase medium, it has been identified in comets and …
A systematic metallicity study of DustPedia galaxies reveals evolution in the dust-to-metal ratios
Observations of evolution in the dust-to-metal ratio allow us to constrain the dominant dust
processing mechanisms. In this work, we present a study of the dust-to-metal and dust-to …
processing mechanisms. In this work, we present a study of the dust-to-metal and dust-to …
Transition of the initial mass function in the metal-poor environments
S Chon, K Omukai, R Schneider - Monthly Notices of the Royal …, 2021 - academic.oup.com
We study star cluster formation in a low-metallicity environment using three-dimensional
hydrodynamic simulations. Starting from a turbulent cloud core, we follow the formation and …
hydrodynamic simulations. Starting from a turbulent cloud core, we follow the formation and …
[图书][B] Dust in the galactic environment
DCB Whittet - 2018 - taylorfrancis.com
Dust is a ubiquitous feature of the cosmos, impinging directly or indirectly on most fields of
modern astronomy and astrophysics. Dust in the Galactic Environment, Second Edition …
modern astronomy and astrophysics. Dust in the Galactic Environment, Second Edition …
An empirical study of dust properties at the earliest epochs
We present an empirical analysis of the properties of dust-continuum emission in a sample
of 17 galaxies in the early Universe (4< z< 8) with well-sampled far-infrared spectral energy …
of 17 galaxies in the early Universe (4< z< 8) with well-sampled far-infrared spectral energy …
The assembly of dusty galaxies at z ≥ 4: the build-up of stellar mass and its scaling relations with hints from early JWST data
The increasing number of distant galaxies observed with ALMA by the ALPINE and REBELS
surveys and the early release observations of the JWST promise to revolutionize our …
surveys and the early release observations of the JWST promise to revolutionize our …
The assembly of dusty galaxies at z ≥ 4: statistical properties
The recent discovery of high-redshift dusty galaxies implies a rapid dust enrichment of their
interstellar medium (ISM). To interpret these observations, we run a cosmological simulation …
interstellar medium (ISM). To interpret these observations, we run a cosmological simulation …
Observed cosmic evolution of galaxy dust properties with metallicity and tensions with models
G Popping, C Péroux - Monthly Notices of the Royal …, 2022 - academic.oup.com
The dust abundance of the interstellar medium plays an important role in galaxy physics, the
chemical evolution of matter, and the absorption and re-emission of stellar light. The last …
chemical evolution of matter, and the absorption and re-emission of stellar light. The last …