HI4PI: a full-sky H i survey based on EBHIS and GASS

NB Bekhti, L Flöer, R Keller, J Kerp, D Lenz… - Astronomy & …, 2016 - aanda.org
Context. Measurement of the Galactic neutral atomic hydrogen (H i) column density, NH i,
and brightness temperatures, TB, is of high scientific value for a broad range of astrophysical …

[PDF][PDF] HI4PI: A full-sky HI survey based on EBHIS and GASS

N Ben Bekhti, L Flöer, R Keller, DJ Pisano - 2016 - researchrepository.wvu.edu
ABSTRACT Context. Measurement of the Galactic neutral atomic hydrogen (H i) column
density, NH i, and brightness temperatures, TB, is of high scientific value for a broad range of …

Understanding star formation in molecular clouds-IV. Column density PDFs from quiescent to massive molecular clouds

N Schneider, V Ossenkopf-Okada, S Clarke… - Astronomy & …, 2022 - aanda.org
Probability distribution functions of the total hydrogen column density (N-PDFs) are a
valuable tool for distinguishing between the various processes (turbulence, gravity, radiative …

Understanding star formation in molecular clouds-II. Signatures of gravitational collapse of IRDCs

N Schneider, T Csengeri, RS Klessen… - Astronomy & …, 2015 - aanda.org
We analyse column density and temperature maps derived from Herschel dust continuum
observations of a sample of prominent, massive infrared dark clouds (IRDCs) ie G11. 11 …

Constraining the H2 column densities in the diffuse interstellar medium using dust extinction and HI data

R Skalidis, PF Goldsmith, PF Hopkins… - Astronomy & …, 2024 - aanda.org
Context. Carbon monoxide (CO) is a poor tracer of H 2 in the diffuse interstellar medium
(ISM), where most of the carbon is not incorporated into CO molecules, unlike the situation at …

Searching for inflationary B modes: can dust emission properties be extrapolated from 350 GHz to 150 GHz?

K Tassis, V Pavlidou - Monthly Notices of the Royal Astronomical …, 2015 - academic.oup.com
Recent Planck results have shown that radiation from the cosmic microwave background
passes through foregrounds in which aligned dust grains produce polarized dust emission …

Maps of the number of H i clouds along the line of sight at high galactic latitude

GV Panopoulou, D Lenz - The Astrophysical Journal, 2020 - iopscience.iop.org
Characterizing the structure of the Galactic interstellar medium (ISM) in three dimensions is
of high importance for accurate modeling of dust emission as a foreground to the cosmic …

All-sky census of Galactic high-latitude molecular intermediate-velocity clouds

T Röhser, J Kerp, D Lenz, B Winkel - Astronomy & Astrophysics, 2016 - aanda.org
Context. The H i halo clouds of the Milky Way, and in particular the intermediate-velocity
clouds (IVCs), are thought to be connected to Galactic fountain processes. Observations of …

First detection of the [CII] 158 µm line in the intermediate-velocity cloud Draco

N Schneider, V Ossenkopf-Okada, E Keilmann… - Astronomy & …, 2024 - aanda.org
High-latitude intermediate-velocity clouds (IVCs) are part of the Milky Way's HI halo and
originate from either a galactic fountain process or extragalactic gas infall. They are partly …

Limits on the OH Molecule in the Smith High-velocity Cloud

AH Minter, FJ Lockman, SA Balashev… - The Astrophysical …, 2024 - iopscience.iop.org
We have used the Green Bank Telescope to search for the OH molecule at several locations
in the Smith Cloud, one of the most prominent of the high-velocity clouds surrounding the …