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Recent star formation in the Lupus clouds as seen by<i>Herschel</i>

2012· article· en· 52 citations· W1983240562 on OpenAlex· 10.1051/0004-6361/201219511

Why is this work in the frame?

A frame that forgets how it found something cannot be audited. These are the routes that admitted this work.

Canadian affiliationAn author listed a Canadian institution. This is the only route the usual frame has.

The three-model screen

all 1,000 screened works →

All three models called this out of scope.

stratum: aff_core · design weight: 5595.24 (the sample is stratified; any rate computed without the weight is wrong)
Claude Opus 4.8OUT
genre: empirical
about Canada: no
confidence: high

Astrophysical study of star formation in the Lupus clouds.

GPT-5.6 (high)OUT
genre: empirical
about Canada: no
confidence: high

The article studies star formation in molecular clouds, not the conduct of research.

Grok 4.5OUT
genre: empirical
about Canada: no
confidence: high

Astrophysics of star formation in Lupus clouds, domain science.

Abstract

We present a study of the star formation histories of the Lupus I, III, and IV clouds using the Herschel 70–500 μm maps obtained by the Herschel Gould Belt Survey Key Project. By combining the new Herschel data with the existing Spitzer catalog we obtained an unprecedented census of prestellar sources and young stellar objects in the Lupus clouds, which allowed us to study the overall star formation rate (SFR) and efficiency (SFE). The high SFE of Lupus III, its decreasing SFR, and its large number of pre-main sequence stars with respect to proto- and prestellar sources, suggest that Lupus III is the most evolved cloud, and after having experienced a major star formation event in the past, is now approaching the end of its current star-forming cycle. Lupus I is currently undergoing a large star formation event, apparent by the increasing SFR, the large number of prestellar objects with respect to more evolved objects, and the high percentage of material at high extinction (e.g., above AV ≈ 8 mag). Also Lupus IV has an increasing SFR; however, the relative number of prestellar sources is much lower, suggesting that its star formation has not yet reached its peak.

Stored with the screening record, where it is evidence for the labels above.

The record

Venue
Astronomy and Astrophysics
Topic
Astrophysics and Star Formation Studies
Field
Physics and Astronomy
Canadian institutions
Canadian Institute for Theoretical AstrophysicsNational Research Council CanadaUniversity of VictoriaUniversity of TorontoHerzberg Institute of Astrophysics
Funders
Science and Technology Facilities CouncilMax-Planck-Institut für AstronomieCentre National de la Recherche ScientifiqueKU LeuvenNational Aeronautics and Space AdministrationCalifornia Institute of TechnologyImperial College LondonNational Astronomical Observatories, Chinese Academy of SciencesUK Space AgencyCentre National d’Etudes Spatiales
Keywords
Systemic lupus erythematosusStar formationExtinction (optical mineralogy)StarsMolecular cloudStar (game theory)
Has abstract in OpenAlex
yes