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Anomalous nature of outbursts of black hole candidate 4U 1630−472

2021· preprint· en· 0 citations· W3176735787 on OpenAlex· 10.1093/mnras/stab3570

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

Canadian funderA Canadian agency funded it. The work may carry no Canadian affiliation at all.

No Canadian affiliation. An affiliation-only frame — the usual design — would never have seen this work. It is one of the works that make the case for inverting the frame.

The three-model screen

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All three models called this out of scope.

stratum: fund_new · design weight: 1678.90 (the sample is stratified; any rate computed without the weight is wrong)
Claude Opus 4.8OUT
genre: empirical
about Canada: no
confidence: high

X-ray astronomy analysis of outbursts from a Galactic black hole candidate; the object is an astrophysical source.

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

This study analyzes black hole outbursts using astronomical observations, not research itself.

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

Astrophysics of black-hole candidate outbursts; domain physical science.

Abstract

ABSTRACT The Galactic black hole candidate (BHC) 4U 1630−472 has gone through several outbursts (13 to be particular) in the last two and a half decades starting from the RXTE era till date. Like the outbursts of other transient BHCs, the outbursts of this source show variations in duration, peak numbers, highest peak flux, etc. However, unlike other soft X-ray transients, this source showed outbursts of two types, such as normal and super. The normal outbursts of duration ∼100−200 d are observed with an average recurrence or quiescence period of ∼500 d. The super outbursts of duration ∼1.5−2.5 yr, consist of more than one normal outburst and one mega outburst. We make an effort to separate the flux contributions of the normal and mega components from the super outbursts, and try to understand the nature of evolution of both types (normal and mega) of outbursts, based on the quiescent period prior to the outbursts. Archival data of RXTE or ASM from 1996 January to 2011 June, and MAXI or GSC from 2009 August to 2020 July are used for our study. Based on the variations of various properties of both the normal and mega outbursts, we think that this BHC is a special source which may contain two companions. Two companions might be responsible for two types of outbursts.

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

The record

Venue
Monthly Notices of the Royal Astronomical Society
Topic
Astrophysical Phenomena and Observations
Field
Physics and Astronomy
Canadian institutions
Funders
RIKENJapan Aerospace Exploration AgencyUniversity Grants CommissionDepartment of Science and Technology, Republic of South AfricaIndian Space Research OrganisationInspire FoundationCanada's Michael Smith Genome Sciences CentreCouncil for Scientific and Industrial Research, South AfricaAmerican Society for MicrobiologyNational Aeronautics and Space Administration
Keywords
AstrophysicsPhysicsFlux (metallurgy)Black hole (networking)Duration (music)Astronomy
Has abstract in OpenAlex
yes