eCite Digital Repository

Small-scale structure traced by neutral hydrogen absorption in the direction of multiple-component radio continuum sources

Citation

Rybarczyk, DR and Stanimirovic, S and Zweibel, EG and Murray, CE and Dickey, JM and Babler, B and Heiles, C, Small-scale structure traced by neutral hydrogen absorption in the direction of multiple-component radio continuum sources, Astrophysical Journal, 893, (2) pp. 1-21. ISSN 0004-637X (2020) [Refereed Article]


Preview
PDF
Pending copyright assessment - Request a copy
2Mb
  

DOI: doi:10.3847/1538-4357/ab83f7

Abstract

We have studied the small-scale distribution of atomic hydrogen (H i) using 21 cm absorption spectra against multiple-component background radio continuum sources from the 21-SPONGE survey and the Millennium Arecibo Absorption-Line Survey. We have found >5 sigma optical depth variations at a level of similar to 0.03-0.5 between 13 out of 14 adjacent sightlines separated by a few arcseconds to a few arcminutes, suggesting the presence of neutral structures on spatial scales from a few to thousands of au (which we refer to as tiny-scale atomic structure, TSAS). The optical depth variations are strongest in directions where the H i column density and the fraction of H i in the cold neutral medium (CNM) are highest, which tend to be at low Galactic latitudes. By measuring changes in the properties of Gaussian components fitted to the absorption spectra, we find that changes in both the peak optical depth and the linewidth of TSAS absorption features contribute to the observed optical depth variations, while changes in the central velocity do not appear to strongly impact the observed variations. Both thermal and turbulent motions contribute appreciably to the linewidths, but the turbulence does not appear strong enough to confine overpressured TSAS. In a majority of cases, the TSAS column densities are sufficiently high that these structures can radiatively cool fast enough to maintain thermal equilibrium with their surroundings, even if they are overpressured. We also find that a majority of TSAS is associated with the CNM. For TSAS in the direction of the Taurus molecular cloud and the local Leo cold cloud, we estimate densities over an order of magnitude higher than typical CNM densities.

Item Details

Item Type:Refereed Article
Keywords:neutral hydrogen clouds, interstellar medium, interstellar line absorption, Milky Way Galaxy
Research Division:Physical Sciences
Research Group:Astronomical sciences
Research Field:Galactic astronomy
Objective Division:Expanding Knowledge
Objective Group:Expanding knowledge
Objective Field:Expanding knowledge in the physical sciences
UTAS Author:Dickey, JM (Professor John Dickey)
ID Code:152800
Year Published:2020
Web of Science® Times Cited:5
Deposited By:Mathematics
Deposited On:2022-08-24
Last Modified:2022-08-24
Downloads:0

Repository Staff Only: item control page