about
Light curves of the neutron star merger GW170817/SSS17a: Implications for r-process nucleosynthesis.The r-process Pattern of a Bright, Highly r-process-enhanced Metal-poor Halo Star at [Fe/H] ∼ −2Hubble Space Telescope near-ultraviolet spectroscopy of bright CEMP-s starsAn elemental assay of very, extremely, and ultra-metal-poor starsExploring the origin of lithium, carbon, strontium, and barium with four new ultra metal-poor starsThe binary frequency of r-process-element-enhanced metal-poor stars and its implications: chemical tagging in the primitive halo of the Milky wayThe R-Process Alliance: First Release from the Northern Search for r-process-enhanced Metal-poor Stars in the Galactic Halo
P50
Q46867247-36F483EB-F71D-4862-91AB-4D8DDC514726Q56958540-36ADA0ED-501E-4C23-8206-D78F21D388E7Q56958611-F5101443-A429-4252-8CC5-4FA72E6090B6Q56958636-714FDF0F-CBA8-434A-A619-1D6638B49E8FQ56958688-C1F87554-A5E7-4729-BAD0-213AF5C76D17Q59743853-5B282BC4-CA8F-4B12-9BEE-D17AF5EBFDBBQ60168089-B0EEB7C2-FDCD-47D2-BE14-4780C528019D
P50
description
onderzoeker
@nl
researcher
@en
հետազոտող
@hy
name
Terese Hansen
@ast
Terese Hansen
@en
Terese Hansen
@es
Terese Hansen
@nl
type
label
Terese Hansen
@ast
Terese Hansen
@en
Terese Hansen
@es
Terese Hansen
@nl
prefLabel
Terese Hansen
@ast
Terese Hansen
@en
Terese Hansen
@es
Terese Hansen
@nl
P106
P31
P496
0000-0001-6154-8983