SwePub
Sök i LIBRIS databas

  Extended search

id:"swepub:oai:research.chalmers.se:ab237aaf-bcc2-4150-b440-b2569b9543db"
 

Search: id:"swepub:oai:research.chalmers.se:ab237aaf-bcc2-4150-b440-b2569b9543db" > A closer look at th...

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist

A closer look at the `characteristic' width of molecular cloud filaments

Panopoulou, Georgia, 1989 (author)
Panepistimio Kritis,University of Crete
al., et (author)
 (creator_code:org_t)
2016-11-23
2017
English.
In: Monthly Notices of the Royal Astronomical Society. - : Oxford University Press (OUP). - 0035-8711 .- 1365-2966. ; 466:3, s. 2529-2541
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • Filaments in Herschel molecular cloud images are found to exhibit a 'characteristic width'. This finding is in tension with spatial power spectra of the data, which show no indication of this characteristic scale. We demonstrate that this discrepancy is a result of the methodology adopted for measuring filament widths. First, we perform the previously used analysis technique on artificial scale-free data, and obtain a peaked width distribution of filament-like structures. Next, we repeat the analysis on three Herschel maps and reproduce the narrow distribution of widths found in previous studies - when considering the average width of each filament. However, the distribution of widths measured at all points along a filament spine is broader than the distribution of mean filament widths, indicating that the narrow spread (interpreted as a 'characteristic' width) results from averaging. Furthermore, the width is found to vary significantly from one end of a filament to the other. Therefore, the previously identified peak at 0.1 pc cannot be understood as representing the typical width of filaments. We find an alternative explanation by modelling the observed width distribution as a truncated power-law distribution, sampled with uncertainties. The position of the peak is connected to the lower truncation scale and is likely set by the choice of parameters used in measuring filament widths. We conclude that a 'characteristic' width of filaments is not supported by the available data.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

stars: formation
ISM: individual objects: Polaris Flare
Astrophysics - Astrophysics of Galaxies
ISM: individual objects: IC 5146
Astrophysics - Solar and Stellar Astrophysics
ISM: individual objects: Aquila Rift
methods: statistical
ISM: clouds

Publication and Content Type

art (subject category)
ref (subject category)

Find in a library

To the university's database

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist

Find more in SwePub

By the author/editor
Panopoulou, Geor ...
al., et
About the subject
NATURAL SCIENCES
NATURAL SCIENCES
and Physical Science ...
and Astronomy Astrop ...
Articles in the publication
Monthly Notices ...
By the university
Chalmers University of Technology

Search outside SwePub

Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.

 
pil uppåt Close

Copy and save the link in order to return to this view