Vinicius Placco astronomer
Placco, Vinicius M.
VIAF ID: 3374151112571537180005 (Personal)
Permalink: http://viaf.org/viaf/3374151112571537180005
Preferred Forms
- 100 1 _ ‡a Placco, Vinicius M.
- 100 0 _ ‡a Vinicius Placco ‡c astronomer
4xx's: Alternate Name Forms (5)
5xx's: Related Names (4)
- 510 2 _ ‡a American Astronomical Society ‡4 rela ‡4 https://d-nb.info/standards/elementset/gnd#relatedCorporateBody ‡e Relation allgemein
- 510 2 _ ‡a Brazilian Astronomical Society ‡4 rela ‡4 https://d-nb.info/standards/elementset/gnd#relatedCorporateBody ‡e Relation allgemein
- 510 2 _ ‡a Gemini Observatory Users Committee ‡4 affi ‡4 https://d-nb.info/standards/elementset/gnd#affiliation ‡e Affiliation
- 510 2 _ ‡a Sociedade Brasileira de Física ‡4 rela ‡4 https://d-nb.info/standards/elementset/gnd#relatedCorporateBody ‡e Relation allgemein
Works
Title | Sources |
---|---|
2MASS J18082002−5104378: The brightest | |
Abundance analysis of APOGEE spectra for 58 metal-poor stars from the bulge spheroid | |
Bright metal-poor stars from the Hamburg/ESO Survey. II. A chemodynamical analysis | |
Carbon-enhanced metal-poor star frequencies in the galaxy: corrections for the effect of evolutionary status on carbon abundances | |
The case for electron re-acceleration at galaxy cluster shocks | |
<i>Chandra</i> Observations of the Spectacular A3411–12 Merger Event | |
The Chemical Abundances of Stars in the Halo (CASH) Project. III. A new classification scheme for carbon-enhanced metal-poor stars with s-process element enhancement | |
Early spectra of the gravitational wave source GW170817: Evolution of a neutron star merger. | |
Element abundance patterns in stars indicate fission of nuclei heavier than uranium | |
Evidence for an Aspherical Population III Supernova Explosion Inferred from the Hyper-metal-poor Star HE 1327–2326 | |
HUBBLE SPACE TELESCOPENEAR-ULTRAVIOLET SPECTROSCOPY OF BRIGHT CEMP-sSTARS | |
IDENTIFICATION OF NEODYMIUM IN THE APOGEEH-BAND SPECTRA | |
Metal-poor Stars Observed with the Automated Planet Finder Telescope. I. Discovery of Five Carbon-enhanced Metal-poor Stars from LAMOST | |
METAL-POOR STARS OBSERVED WITH THE MAGELLAN TELESCOPE. I. CONSTRAINTS ON PROGENITOR MASS AND METALLICITY OF AGB STARS UNDERGOINGs-PROCESS NUCLEOSYNTHESIS | |
METAL-POOR STARS OBSERVED WITH THEMAGELLANTELESCOPE. III. NEW EXTREMELY AND ULTRA METAL-POOR STARS FROM SDSS/SEGUE AND INSIGHTS ON THE FORMATION OF ULTRA METAL-POOR STARS | |
The Origin of the 300 km s−1 Stream near Segue 1 | |
Population studies. XIII. A new analysis of the Bidelman-MacConnell "weak-metal" Stars--Confirmation of metal-poor stars in the thick disk of the galaxy | |
The R-Process Alliance: A Comprehensive Abundance Analysis of HD 222925, a Metal-poor Star with an Extreme R-process Enhancement of [Eu/H] = −0.14 | |
The R-Process Alliance: Chemical Abundances for a Trio of r-process-enhanced Stars—One Strong, One Moderate, and One Mild | |
The R-Process Alliance: Discovery of the First Metal-poor Star with a Combined r- and s-process Element Signature | |
The R-process Alliance: First Release from the Southern Search for R-process-enhanced Stars in the Galactic Halo | |
The R-Process Alliance: Spectroscopic Follow-up of Low-metallicity Star Candidates from the Best & Brightest Survey | |
The r-process Pattern of a Bright, Highly r-process-enhanced Metal-poor Halo Star at [Fe/H] ∼ −2 | |
RAVE J203843.2–002333: The First Highly R-process-enhanced Star Identified in the RAVE Survey | |
SD 1313–0019: ANOTHER SECOND-GENERATION STAR WITH [Fe/H] = −5.0, OBSERVED WITH THEMAGELLANTELESCOPE |