0000000000338103

AUTHOR

Birgitta Nordström

showing 4 related works from this author

The Hamburg/ESO R-process Enhanced Star survey (HERES)

2004

We report on a dedicated effort to identify and study metal-poor stars strongly enhanced in r-process elements ([r/Fe] > 1 dex; hereafter r-II stars), the Hamburg/ESO R-process Enhanced Star survey (HERES). Moderate-resolution (~2A) follow-up spectroscopy has been obtained for metal-poor giant candidates selected from the Hamburg/ESO objective-prism survey (HES) as well as the HK survey to identify sharp-lined stars with [Fe/H] < -2.5dex. For several hundred confirmed metal-poor giants brighter than B~16.5mag (most of them from the HES), ``snapshot'' spectra (R~20,000; S/N~30 per pixel) are being obtained with VLT/UVES, with the main aim of finding the 2-3% r-II stars expected to be a…

population II [stars]PhysicsAstrophysics (astro-ph)FOS: Physical sciencesabundances [Galaxy]Astronomy and AstrophysicsAstrophysicsStar (graph theory)AstrophysicsSpectral lineabundances [stars]Neutron captureStarssurveysSpace and Planetary SciencePhenomenological modelhalo [Galaxy]Astronomy Astrophysics and Cosmologyr-processSpectroscopyRadioactive decayAstronomy & Astrophysics
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The Hamburg/ESO R-process Enhanced Star survey (HERES): Project Overview, and New r-II Stars

2005

PhysicsStarsSpiral galaxySpace and Planetary ScienceIntergalactic starAstronomyr-processAstronomy and AstrophysicsStar countAstrophysicsStar (graph theory)GalaxyDwarf galaxyProceedings of the International Astronomical Union
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The Hamburg/ESO R-process Enhanced Star survey (HERES):XI. The highly r-process-enhanced star CS 29497-004

2017

We report an abundance analysis for the highly r-process-enhanced (r-II) star CS 29497-004, a very metal-poor giant with Teff = 5013K and [Fe/H]=-2.85, whose nature was initially discovered in the course of the HERES project. Our analysis is based on high signal-to-noise, high-resolution (R~75000) VLT/UVES spectra and MARCS model atmospheres under the assumption of local thermodynamic equilibrium, and obtains abundance measurements for a total of 46 elements, 31 of which are neutron-capture elements. As is the case for the other 25 r-II stars currently known, the heavy-element abundance pattern of CS 29497-004 well-matches a scaled Solar System second peak r-process-element abundance patter…

MODEL ATMOSPHERESSolar SystemPopulation II [stars]Thermodynamic equilibriumMETAL-POOR STARSFOS: Physical sciencesAstrophysicsStar (graph theory)01 natural sciences7. Clean energySpectral lineGalactic halochemically peculiar [stars]CORE-COLLAPSE SUPERNOVAELABORATORY TRANSITION-PROBABILITIES0103 physical sciencesEXPERIMENTAL OSCILLATOR-STRENGTHShalo [Galaxy]NeutronEARLY GALAXY010306 general physics010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSSolar and Stellar Astrophysics (astro-ph.SR)PhysicsPROCESS-RICHGALACTIC CHEMICAL EVOLUTIONAstronomy and Astrophysicsindividual: CS 29497-004 [stars][PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]Astrophysics - Astrophysics of Galaxiesabundances [stars]StarsHIGH-ENTROPY-WIND[PHYS.ASTR.GA]Physics [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA]Astrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)r-processNEUTRON-CAPTURE
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Women Scientists Who Made Nuclear Astrophysics

2019

Female role models reduce the impact on women of stereotype threat, i.e. of being at risk of conforming to a negative stereotype about one’s social, gender, or racial group (Fine in Delusion of Gender. W.W. Norton & Co. NY, p. 36, 2010 [1]; Steele and Aronson in J Pers Soc Psychol 69:797–811, 1995 [2]). This can lead women scientists to underperform or to leave their scientific career because of negative stereotypes such as, not being as talented or as interested in science as men. Sadly, history rarely provides role models for women scientists; instead, it often renders these women invisible (CafeBabel Homepage [3]). In response to this situation, we present a selection of twelve outst…

naisetFissionNuclear TheoryAstronomyNuclear physics050109 social psychologykosmologiaAstrophysics01 natural sciencestähtitiedeSolar studies5. Gender equalityHistory and Philosophy of Physics (physics.hist-ph)Nuclear Experiment (nucl-ex)Nuclear Experiment010303 astronomy & astrophysicsNuclear theoryQCQBEarth and Planetary Astrophysics (astro-ph.EP)High Energy Astrophysical Phenomena (astro-ph.HE)Women scientistsHistorical05 social sciencesGender studiestutkijatCosmologyStereotype threatRadioactivityAstrophysics - Solar and Stellar Astrophysicsmedicine.symptomAstrophysics - High Energy Astrophysical PhenomenaPsychologyydinfysiikkaScientific careerastrofysiikkaeducationPhysics - History and Philosophy of PhysicsFOS: Physical sciencesNegative stereotypeNuclear Theory (nucl-th)Delusion0103 physical sciencesmedicine0501 psychology and cognitive sciencesSolar and Stellar Astrophysics (astro-ph.SR)radioaktiivisuusRacial groupGénéralitésAstrophysics - Astrophysics of GalaxiesfissioAstrophysics of Galaxies (astro-ph.GA)Astrophysics - Earth and Planetary Astrophysics
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