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19992023
most citedGalactic chemical evolution: Carbon through Zinc

890 citations · 8.7k across the 111 of their papers we have counts for

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Showing 2017Show all

6 papers · 1 filter

astro-ph.SR2017★ 60 cited

Constraining cosmic scatter in the Galactic halo through a differential analysis of metal-poor stars

Henrique Reggiani, Jorge Meléndez, Chiaki Kobayashi +2

We present the abundances of Li, Na, Mg, Al, Si, Ca, Sc, Ti, V, Cr, Mn, Co, Ni, Zn, Sr, Y, Zr, and Ba in a wide metallicity range ( [Fe/H] ). Using the differen…

astro-ph.GA2017★ 22 cited

Manganese spread in Ursa Minor as a proof of sub-classes of type Ia supernovae

Gabriele Cescutti, Chiaki Kobayashi

Context. Recently, new sub-classes of Type Ia supernovae (SNe Ia) were discovered, including SNe Iax. The suggested progenitors of SNe Iax are relatively massive, possibly hybrid C…

astro-ph.GA2017★ 87 cited

The Chemical Evolution Carousel of Spiral Galaxies: Azimuthal Variations of Oxygen Abundance in NGC1365

I-Ting Ho, Mark Seibert, Sharon E. Meidt +9

The spatial distribution of oxygen in the interstellar medium of galaxies is the key to understanding how efficiently metals that are synthesized in massive stars can be redistribu…

astro-ph.GA2017

The chemical signature of SNIax in the stars of Ursa minor?

G. Cescutti, C. Kobayashi

Recently, a new class of supernovae Ia was discovered: the supernovae Iax; the increasing sample of these objects share common features as lower maximum-light velocities and typica…

astro-ph.GA2017★ 55 cited

The Metallicity and Elemental Abundance Gradients of Simulated Galaxies, and their Environmental Dependence

Philip Taylor, Chiaki Kobayashi

The internal distribution of heavy elements, in particular the radial metallicity gradient, offers insight into the merging history of galaxies. Using our cosmological, chemodynami…

astro-ph.GA2017★ 16 cited

Star Formation in Simulated Galaxies: Understanding the Transition to Quiescence at M

Philip Taylor, Christoph Federrath, Chiaki Kobayashi

Star formation in galaxies relies on the availability of cold, dense gas, which, in turn, relies on factors internal and external to the galaxies. In order to provide a simple mode…