A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE)-I. Introduction to the survey
A Boselli, M Fossati, L Ferrarese, S Boissier… - Astronomy & …, 2018 - aanda.org
The Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) is a blind narrow-
band (NB) Hα+[NII] imaging survey carried out with MegaCam at the Canada–France …
band (NB) Hα+[NII] imaging survey carried out with MegaCam at the Canada–France …
Quantifying the energy balance between the turbulent ionised gas and young stars
OV Egorov, K Kreckel, SCO Glover, B Groves… - Astronomy & …, 2023 - aanda.org
Context. Stellar feedback is a key contributor to the morphology and dynamics of the
interstellar medium in star-forming galaxies. In particular, energy and momentum input from …
interstellar medium in star-forming galaxies. In particular, energy and momentum input from …
A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE)-IX. The effects of ram pressure stripping down to the scale of individual HII regions in the …
We study the IB (s) m galaxy IC 3476 observed in the context of the Virgo Environmental
Survey Tracing Ionised Gas Emission (VESTIGE), a blind narrow-band Hα+[NII] imaging …
Survey Tracing Ionised Gas Emission (VESTIGE), a blind narrow-band Hα+[NII] imaging …
Towards a multitracer timeline of star formation in the LMC–II. The formation and destruction of molecular clouds
JL Ward, JMD Kruijssen, M Chevance… - Monthly Notices of …, 2022 - academic.oup.com
The time-scales associated with various stages of the star formation process represent major
unknowns in our understanding of galactic evolution, as well as of star and planet formation …
unknowns in our understanding of galactic evolution, as well as of star and planet formation …
Formation of the active star-forming region LHA 120-N 44 triggered by tidally driven colliding H i flows
K Tsuge, H Sano, K Tachihara, C Yozin… - The Astrophysical …, 2019 - iopscience.iop.org
The second most active site of high-mass star formation next to R136 in the Large
Magellanic Cloud (LMC) is N44. We carried out a detailed analysis of H i at 60''resolution by …
Magellanic Cloud (LMC) is N44. We carried out a detailed analysis of H i at 60''resolution by …
Emission-line velocity, metallicity, and extinction maps of the Large Magellanic Cloud
P Lah, M Colless, F D'Eugenio… - Monthly Notices of the …, 2024 - academic.oup.com
We measure the properties of optical emission lines in multiple locations across the Large
Magellanic Cloud (LMC) using the Australian National University 2.3-m telescope and the …
Magellanic Cloud (LMC) using the Australian National University 2.3-m telescope and the …
Evidence of particle acceleration in the superbubble 30 doradus c with NuSTAR
We present evidence of diffuse, non-thermal X-ray emission from the superbubble 30
Doradus C (30 Dor C) using hard X-ray images and spectra from NuSTAR observations. For …
Doradus C (30 Dor C) using hard X-ray images and spectra from NuSTAR observations. For …
High-mass star formation in the Large Magellanic Cloud triggered by colliding H i flows
The galactic tidal interaction is a possible mechanism to trigger active star formation in
galaxies. Recent analyses using H i data in the Large Magellanic Cloud (LMC) proposed …
galaxies. Recent analyses using H i data in the Large Magellanic Cloud (LMC) proposed …
Kinematics and Feedback in H II regions in the Dwarf Starburst Galaxy IC 10
We present a survey of the central region of the nearest starburst galaxy, IC 10, using the
WM Keck Observatory Keck Cosmic Web Imager (KCWI) at high spectral and spatial …
WM Keck Observatory Keck Cosmic Web Imager (KCWI) at high spectral and spatial …
MaNGA galaxies with off-centered spots of enhanced gas velocity dispersion
Off-centered spots of the enhanced gas velocity dispersion, σ, are revealed in some galaxies
from the Mapping Nearby Galaxies at Apache Point Observatory survey (MaNGA). Aiming to …
from the Mapping Nearby Galaxies at Apache Point Observatory survey (MaNGA). Aiming to …