A Catalog of Filaments in the Central Molecular Zone

Abstract We present a catalog of 1.28 GHz radio filaments observed by MeerKAT over the innermost 200 pc of the Galaxy (roughly ±1 <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mover> <mml:mrow> <mml:mo>.</mml:mo> </mml:mrow> <mml:mrow> <mml:mtext>°</mml:mtext> </mml:mrow> </mml:mover> </mml:math> 5), which includes the central molecular zone. The catalog is generated by repurposing software developed for the automated detection of filaments in solar coronal loops. There are two parts to the catalog. The first part, the main catalog, provides a point-by-point listing of locations and basic observational properties along each detected filament. The second part is a summary catalog that provides a listing of mean, median, or total values of various properties for each filament. Tabulated quantities include position, length, curvature, brightness, and spectral index. The catalogs contain a heterogeneous mix of filamentary structures, including nonthermal radio filaments, and parts of supernova remnants and thermally emitting regions (e.g., H ii regions). We discuss criteria for selecting useful subsamples of filaments from the catalogs, and some of the details encountered in examining filaments or selections of filaments from the catalogs.

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Journal
The Astrophysical Journal Supplement Series
Published
2025-11-13
DOI
https://doi.org/10.3847/1538-4365/ae1296
Primary Topic
Astrophysics and Star Formation Studies
Type
article
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article

A Catalog of Filaments in the Central Molecular Zone

F. Yusef‐Zadeh, Ian Heywood, Richard G. Arendt
The Astrophysical Journal Supplement Series
Astrophysics and Star Formation Studies
article

A Catalog of Filaments in the Central Molecular Zone

F. Yusef‐Zadeh, Ian Heywood, Richard G. Arendt
article en

Abstract

Abstract We present a catalog of 1.28 GHz radio filaments observed by MeerKAT over the innermost 200 pc of the Galaxy (roughly ±1 <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mover> <mml:mrow> <mml:mo>.</mml:mo> </mml:mrow> <mml:mrow> <mml:mtext>°</mml:mtext> </mml:mrow> </mml:mover> </mml:math> 5), which includes the central molecular zone. The catalog is generated by repurposing software developed for the automated detection of filaments in solar coronal loops. There are two parts to the catalog. The first part, the main catalog, provides a point-by-point listing of locations and basic observational properties along each detected filament. The second part is a summary catalog that provides a listing of mean, median, or total values of various properties for each filament. Tabulated quantities include position, length, curvature, brightness, and spectral index. The catalogs contain a heterogeneous mix of filamentary structures, including nonthermal radio filaments, and parts of supernova remnants and thermally emitting regions (e.g., H ii regions). We discuss criteria for selecting useful subsamples of filaments from the catalogs, and some of the details encountered in examining filaments or selections of filaments from the catalogs.

The Astrophysical Journal Supplement SeriesVol. 281(2)
Northwestern University (US), Goddard Space Flight Center (US), Rhodes University (ZA), SKA Observatory (GB), South African Radio Astronomy Observatory (ZA), University of Maryland, Baltimore County (US)
Openalex Percentile: Top 76%
Astrophysics and Star Formation Studies
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