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Record W3167607845 · doi:10.1051/0004-6361/202141294

CAPOS: The bulge Cluster APOgee Survey

2021· article· en· W3167607845 on OpenAlexfundno aff
Marı́a Romero-Colmenares, José G. Fernández-Trincado, D. Geisler, S. O. Souza, S. Villanova, Penélope Longa-Peña, D. Minniti, Timothy C. Beers, C. Moni Bidin, Ángeles Pérez-Villegas, E. Moreno, Elisa R. Garro, Ian Baeza, Lady Henao, B. Barbuy, J. Alonso-García, Roger E. Cohen, Richard R. Lane

Bibliographic record

VenueAstronomy and Astrophysics · 2021
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsnot available
FundersCHIST-ERALawrence Berkeley National LaboratoryAgencia Estatal de InvestigaciónComisión Nacional de Investigación Científica y TecnológicaOffice of ScienceUniversity of Colorado BoulderCarnegie Institution for ScienceInstituto de Astrofísica de CanariasMax-Planck-Institut für AstronomieMax-Planck-Institut für AstrophysikAgencia Nacional de Investigación y DesarrolloDirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de MéxicoJohns Hopkins UniversityInnovációs és Technológiai MinisztériumNemzeti Kutatási Fejlesztési és Innovációs HivatalFinanciadora de Estudos e ProjetosMinisterio de Ciencia, Innovación y UniversidadesMinistério da Ciência, Tecnologia, Inovações e ComunicaçõesCoordenação de Aperfeiçoamento de Pessoal de Nível SuperiorUniversidad Nacional Autónoma de MéxicoMagyar Tudományos AkadémiaConselho Nacional de Desenvolvimento Científico e TecnológicoCarnegie Institution of WashingtonSun Yat-sen UniversityYork UniversityMinistério da Ciência, Tecnologia e InovaçãoFundação de Amparo à Pesquisa do Estado de São PauloLeibniz-GemeinschaftAgence Nationale de la RechercheUniversity of OxfordNational Research, Development and Innovation OfficeAgenția Națională pentru Cercetare și DezvoltareEuropean Regional Development FundCentre National de la Recherche ScientifiqueUniversity of Notre DameJoint Institute for Nuclear Astrophysics - Center for the Evolution of the ElementsBanco SantanderCarnegie Mellon UniversityAlfred P. Sloan FoundationUniversity of WashingtonSmithsonian Astrophysical ObservatoryEuropean Space AgencyUniversity of UtahNew Mexico State UniversityUniversity of PortsmouthInstituto MilleniumVanderbilt UniversityU.S. Department of EnergyYale UniversityDeutsche ForschungsgemeinschaftDepartamento Administrativo de Ciencia, Tecnología e Innovación (COLCIENCIAS)National Natural Science Foundation of ChinaOhio State UniversityNational Science FoundationUniversidad de AntofagastaSmithsonian Institution
KeywordsPhysicsAstrophysicsGlobular clusterBulgeMetallicityDwarf galaxyAstronomyGalaxyPopulationRed-giant branchStarsStar clusterCluster (spacecraft)Dwarf spheroidal galaxyInteracting galaxy

Abstract

fetched live from OpenAlex

We present results from a study of 15 red giant members of the intermediate-metallicity globular cluster (GC) FSR 1758 using high-resolution, near-infrared spectra collected with the Apache Point Observatory Galactic Evolution Experiment II survey (APOGEE-2) that were obtained as part of CAPOS (the bulge Cluster APOgee Survey). Since its very recent discovery as a massive GC in the bulge region, evoking the name Sequoia, this has been an intriguing object with a highly debated origin, and initially led to the suggestion of a purported progenitor dwarf galaxy of the same name. In this work, we use new spectroscopic and astrometric data to provide additional clues as to the nature of FSR 1758. Our study confirms the GC nature of FSR 1758, and as such we report the existence of the characteristic N-C anticorrelation and Al-N correlation for the first time. We thereby reveal the existence of the multiple-population phenomenon, similar to that observed in virtually all GCs. Furthermore, the presence of a population with strongly enriched aluminum makes it unlikely that FSR 1758 is the remnant nucleus of a dwarf galaxy because Al-enhanced stars are uncommon in dwarf galaxies. We find that FSR 1758 is slightly more metal rich than previously reported in the literature; this source has a mean metallicity [Fe/H] between −1.43 to −1.36, depending on the adopted atmospheric parameters and a scatter within observational error, again pointing to its GC nature. Overall, the α-enrichment (≳ + 0.3 dex), Fe-peak (Fe, Ni), light (C, N), and odd-Z (Al) elements follow the trend of intermediate-metallicity GCs. Isochrone fitting in the Gaia bands yields an estimated age of ∼11.6 Gyr. We used the exquisite kinematic data, including our CAPOS radial velocities and Gaia eDR3 proper motions, to constrain the N-body density profile of FSR 1758, and found that it is as massive (∼2.9 ± 0.6 × 105 M⊙) as NGC 6752. We confirm a retrograde and eccentric orbit for FSR 1758. A new examination of its dynamical properties with the GravPot16 model favors an association with the Gaia-Enceladus-Sausage accretion event. Thus, paradoxically, the cluster that gave rise to the name of the Sequoia dwarf galaxy does not appear to belong to this specific merging event.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.042
Threshold uncertainty score0.083

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0030.003
Science and technology studies0.0010.000
Scholarly communication0.0010.000
Open science0.0010.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0030.001

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.012
GPT teacher head0.211
Teacher spread0.199 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations23
Published2021
Admission routes1
Has abstractyes

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