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Lista de obras de Terese Hansen

Abundances of carbon-enhanced metal-poor stars as constraints on their formation

artículo científico publicado en 2016

An elemental assay of very, extremely, and ultra-metal-poor stars

artículo científico publicado en 2015

Birds of a Feather? Magellan/IMACS Spectroscopy of the Ultra-faint Satellites Grus II, Tucana IV, and Tucana V

Element abundance patterns in stars indicate fission of nuclei heavier than uranium

artículo científico publicado en 2023

Exploring the origin of lithium, carbon, strontium, and barium with four new ultra metal-poor stars

scientific article published in the Astrophysical Journal

HAT-P-50b, HAT-P-51b, HAT-P-52b, and HAT-P-53b: Three Transiting Hot Jupiters and a Transiting Hot Saturn From the HATNet Survey

scientific article published in Astronomical Journal

Hubble Space Telescope near-ultraviolet spectroscopy of bright CEMP-s stars

artículo científico publicado en 2015

Light curves of the neutron star merger GW170817/SSS17a: Implications for r-process nucleosynthesis.

artículo científico publicado en 2017

Metallicities for more than 10 million stars derived from <i>Gaia</i> BP/RP spectra

artículo científico publicado en 2024

Spectroscopy of the Young Stellar Association Price-Whelan 1: Origin in the Magellanic Leading Arm and Constraints on the Milky Way Hot Halo

The R-Process Alliance: Chemical Abundances for a Trio of r-process-enhanced Stars—One Strong, One Moderate, and One Mild

scientific article published in the Astrophysical Journal

The R-Process Alliance: Discovery of a Low-α, r-process-enhanced Metal-poor Star in the Galactic Halo

The R-Process Alliance: First Release from the Northern Search for r-process-enhanced Metal-poor Stars in the Galactic Halo

artículo científico publicado en 2018

The binary frequency of r-process-element-enhanced metal-poor stars and its implications: chemical tagging in the primitive halo of the Milky way

The r-process Pattern of a Bright, Highly r-process-enhanced Metal-poor Halo Star at [Fe/H] ∼ −2