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    <identifier>10.57760/sciencedb.29792</identifier>
    <datestamp>2026-03-16T15:50:42Z</datestamp>
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<oai_dc:dc xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
  <dc:date>2026-03-16</dc:date>
  <dc:title>Galactic Large-scale Filaments Resident in Asymmetric Environments: Clues from Cross-filament Profiles of Density and Temperature</dc:title>
  <dc:identifier>doi:10.57760/sciencedb.29792</dc:identifier>
  <dc:language>en</dc:language>
  <dc:description>The basic parameters, the extracted molecular hydrogen column density (N(H2)) and dust temperature (Td) radial profiles of the 35 Galactic large-scale filaments involved in the paper &amp;quot;Galactic Large-scale Filaments Resident in Asymmetric Environments: Clues from Cross-filament Profiles of Density and Temperature&amp;quot; (DOI: 10.3847/1538-4357/ae3c03).&amp;quot;fil_list.txt&amp;quot;: basic physical parameters of the filaments. Meanings of the columns are: (1) Parental catalog; (2) Filament ID in their parental catalog; (3) Galactic longitude; (4) Galactic latitude; (5) Line of sight velocity; (6) Distance; (7) Velocity gradient; (8)-(9) Minimum and maximum temperature; (10) Mass; (11) Averaged N(H2); (12) Linearity; (13) Morphology; (14) Filament width, obtained by Plummer-like fitting of the molecular hydrogen radial profile; (15) Length of the MST filament spine; (16)-(18): segment-length-weighted averaged |1-&amp;alpha;|, and their uncertainties; (19)-(20): fasy; (21): Length fraction of IAA segments in the filament spine.&amp;quot;G2022_fil&amp;quot;, &amp;quot;W2016_fil&amp;quot;, &amp;quot;W2015_fil&amp;quot;: contain the extracted N(H2) and (Td) radial profiles of each filament.In each folder: (1) &amp;quot;note.txt&amp;quot;: filament name, number of segments in its MST spine, length of the segments. (2) &amp;quot;NH2&amp;quot;: N(H2) radial profile. &amp;quot;sep&amp;quot; and &amp;quot;sep_sig&amp;quot; for the full radial profile, and its uncertainty extracted from a sufficient long region of each segment based on the Herschel Hi-GAL N(H2) maps; &amp;quot;trim&amp;quot; and &amp;quot;trim_sig&amp;quot; for the trimmed radial profile taken into analyzation in the paper. (3) &amp;quot;Td&amp;quot;: similar to &amp;quot;NH2&amp;quot;, the Td radial profiles of each segment extracted from the Hi-GAL Td maps. (4) &amp;quot;xaxis_trim.txt&amp;quot;: x-axis values of the trimmed radial profile.</dc:description>
  <dc:subject>Galaxy; Interstellar Medium; Molecular Clouds; Star Formation</dc:subject>
  <dc:creator>Keyun Su</dc:creator>
  <dc:creator>Ke Wang</dc:creator>
  <dc:creator>Fengwei Xu</dc:creator>
  <dc:creator>N. K. Bhadari</dc:creator>
  <dc:rights>PUBLIC</dc:rights>
  <dc:rights>https://creativecommons.org/licenses/by-nc-nd/4.0/</dc:rights>
  <dc:type>dataset</dc:type>
  <dc:relation>http://www.doi.org/10.3847/1538-4357/ae3c03</dc:relation>
  <dc:publisher>Science Data Bank</dc:publisher>
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