From the 2 of 17 papers with an AI index.
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- James W. Johnson2 profiles3 · h 6
- A. Matthews2 profiles2 · h 26
- Andrew Robertson2 profiles2 · h 3
- C. Observatories2 · h 38
- Department of Astronomy Yale University2 · h 0
- D. Pauli2 · h 8
- J. Bodensteiner2 · h 17
- L. Mahy2 · h 24
- L. Patrick2 profiles2 · h 15
- Melissa K. Ness2 profiles2 · h 5
- M. Gull2 · h 4
- M. López-Morales2 · h 58
- Carnegie Institution for ScienceUS7 papers
- California Institute of TechnologyUS6 papers
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- Center for Astrophysics Harvard & SmithsonianUS4 papers
- Institute of AstronomyRU4 papers
- University of CambridgeGB4 papers
- Astronomical Institute of the Slovak Academy of SciencesSK3 papers
- Astronomy and SpaceAU3 papers
- Flatiron Health (United States)US3 papers
- Flatiron Institute3 papers
- The Ohio State UniversityUS3 papers
- University of Southern CaliforniaUS3 papers
6 papers · 1 filter
Pickles on FIRE: The 3D Shape Evolution of Simulated Milky Way-Mass Galaxies
Luke Y. Xia, Courtney Klein, Jenny D. Wang +6
We use reduced-mass eigentensors to quantify the 3D ellipsoidal shape evolution of thirteen Milky Way-mass galaxies simulated using zoom simulations with FIRE-2 physics; all but on…
The Radio-IR Correlation in the Context of Deep Radio Source Counts
Tirth D. Surti, Vikram Ravi, Allison Matthews +1
Increasingly deep, confusion-limited radio surveys have pushed direct radio source-count measurements down to tens of Jy at 1.4 GHz. Confusion-noise analyses extend the…
The galactic chemical evolution of carbon: Implications for stellar nucleosynthesis
Daniel A. Boyea, James W. Johnson, David H. Weinberg
Carbon (C) is thought to be produced by both core collapse supernovae (CCSN) and asymptotic giant branch (AGB) stars, but the relative contributions of these two sources are uncert…
The chemodynamical memory of a major merger in a NIHAO-UHD Milky Way analogue -- I. A golden thread through time and space
Sven Buder, Tobias Buck, Ãsa Skúladóttir +3
Understanding how past major mergers shaped the Milky Way's present-day structure is a key goal of Galactic archaeology. The Galaxy's chemical and dynamical structure retains the i…
A stellar dynamical mass measurement of an inactive black hole at redshift 2
Andrew B. Newman, Meng Gu, Sirio Belli +34
Supermassive black holes and their host galaxies grow together over time, producing correlations between the black hole mass and various galaxy properties. Determining the evolutio…
Milky Way Mapper decoded abundances -- I. Shared disc enrichment patterns
Melissa K. Ness, Sarah Aquilina, Jennifer Mead +15
Elemental abundances in the Milky Way disc trace its star-formation and enrichment history, but predicting these abundances from theory is limited by uncertain nucleosynthetic yiel…