The formation of very massive stars in early galaxies and implications for intermediate mass black holes

JA Regan, JH Wise, TE Woods, TP Downes… - arXiv preprint arXiv …, 2020 - arxiv.org
We investigate the ab-initio formation of super-massive stars in a pristine atomic cooling
halo. The halo is extracted from a larger self-consistent parent simulation. The halo remains …

Modeling the spectral energy distribution of starburst galaxies-The role of photodissociation regions

P Theulé, D Burgarella, V Buat, M Boquien… - Astronomy & …, 2024 - aanda.org
Context. Analyzing multiwavelength observations of galaxies from the far-ultraviolet to the
millimeter domains provides a wealth of information on the physical properties of galaxies …

Two new nova shells associated with V4362 Sagittarii and DO Aquilae

EJ Harvey, MP Redman, P Boumis… - Monthly Notices of …, 2020 - academic.oup.com
ABSTRACT A classical nova is an eruption on the surface of a white dwarf in an accreting
binary system. The material ejected from the white dwarf surface generally forms an …

Shock shaping? Nebular spectroscopy of nova V906 Carinae

ÉJ Harvey, E Aydi, L Izzo, C Morisset… - Monthly Notices of …, 2023 - academic.oup.com
ABSTRACT V906 Carinae was one of the best observed novae of recent times. It was a
prolific dust producer and harboured shocks in the early evolving ejecta outflow. Here, we …

Recovering the properties of the interstellar medium through integrated spectroscopy: application to the z~ 0 ECO volume-limited star-forming galaxy sample

V Lebouteiller, CT Richardson, MS Polimera… - arXiv preprint arXiv …, 2024 - arxiv.org
Deriving physical parameters from integrated galaxy spectra is paramount to interpret the
cosmic evolution of star formation, chemical enrichment, and energetic sources. We develop …

[引用][C] Decoding the Kinematic and Ionisation Structure of Axisymmetric Nebulae

K Fitzgerald - National University of Ireland …