From the 1 of 21 papers with an AI index.
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- A. Brandeker2 profiles4 · h 34
- H. Osborn2 profiles4 · h 29
- J. V. Loon2 profiles4 · h 22
- Y. Alibert2 profiles4 · h 51
- A. Fortier2 profiles3 · h 3
- A. Leleu2 profiles3 · h 17
- D. Gandolfi3 · h 44
- F. Najarro3 · h 45
- F. Tramper3 · h 24
- G. Scandariato2 profiles3 · h 31
- J. Vink2 profiles3 · h 48
- J. V. van Loon3 · h 21
- Centro de AstrobiologíaES5 papers
- Astronomical Institute of the Slovak Academy of SciencesSK4 papers
- Centre National de la Recherche ScientifiqueFR4 papers
- Heidelberg UniversityDE4 papers
- Institute of AstronomyRU4 papers
- Instituto de Astrofísica de CanariasES4 papers
- Leiden UniversityNL4 papers
- Universidad de La LagunaES4 papers
- University of BernCH4 papers
- Armagh Observatory & PlanetariumGB3 papers
- Astronomy and SpaceAU3 papers
- Australian National UniversityAU3 papers
4 papers · 1 filter
A new Gaia census of OB associations within 1 kpc
Alexis L. Quintana, Nicholas J. Wright, Lilly A. Kormann +6
OB associations are primordial tracers of star formation and Galactic structure. Originally defined about 80 years ago, their historical membership lists have been superseded thank…
Revealing the cold skeleton of the Magellanic Clouds and the Magellanic Bridge with ASKAP
James Dempsey, N. M. McClure-Griffiths, Antoine Marchal +14
We present the GASKAP-HI pilot absorption survey of neutral hydrogen (HI) in the Magellanic system. This survey provides 3219 sightlines across the Large (LMC) and Small Magellanic…
EMU/GAMA: Refining Dust Extinction Corrections for Hα Luminosity Functions Using Radio-Based Calibration
J. Willingham, A. Hopkins, T. Zafar +17
We present a novel approach to correcting H luminosity functions for dust extinction by calibrating against radio-based star formation rates (SFRs), using data from the Evoluti…
The Salamander: A case study of the magnetic field and peculiar morphology of G309.8-2.6 through radio polarimetry
Wenhui Jing, Jennifer L. West, Xiaohui Sun +17
Studying the interaction between core-collapse supernova remnants (SNRs) and their surrounding environments is essential to understanding the mechanism for energy transfer to the i…