The thickness of the HI gas layer in spiral galaxies

Floris Jan Sicking

Research output: Thesis › Thesis fully internal (DIV)

1345 Downloads (Pure)

Abstract

In the present study, in two inclined spiral galaxies, NGC 3198 and NGC 2403, the HI random velocity dispersion and layer thickness will be measured simultaneously. This will be done from the HI velocity dispersion field (the distribution on the sky of the observed HI line of sight velocity dispersion).
Original languageEnglish
QualificationDoctor of Philosophy
Publisher
Publication statusPublished - 1997

Keywords

  • Proefschriften (vorm)
  • Waterstof
  • Interstellair gas
  • Spiraalnevels
  • 39.41

Access to Document

  • titlecon.pdfFinal publisher's version, 57.7 KB
  • c1.pdfFinal publisher's version, 54 KB
  • c2.pdfFinal publisher's version, 179 KB
  • c3.pdfFinal publisher's version, 984 KB
  • c4.pdfFinal publisher's version, 853 KB
  • c5.pdfFinal publisher's version, 393 KB
  • c6.pdfFinal publisher's version, 65.1 KB
  • samenvat.pdfFinal publisher's version, 75.1 KB
  • thesis.pdfFinal publisher's version, 2.53 MB

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