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20012018
most citedThe Spin Temperature of Warm Interstellar H I

145 citations · 309 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2018★ 22 cited

Molecular Gas and Dark Neutral Medium in the Outskirts of Chamaeleon

H. Liszt, M. Gerin, I. Grenier

%context More gas is inferred to be present in molecular cloud complexes than can be accounted for by HI and CO emission, a phenomenon known as dark neutral medium (DNM) or CO-dark…

astro-ph.GA2017★ 11 cited

ALMA observations of molecular absorption in four directions toward the Galactic bulge

H. Liszt, M. Gerin

Alma Cycle 3 observations showed strong absorption from diffuse molecular gas in the bulge at -200 \kms\ \kms\ toward J1744-3116 (l,b)= (-2.13d,-1d) We aimed to…

astro-ph.GA2015★ 10 cited

First Detection of HCO Absorption in the Magellanic System

Claire E. Murray, Snežana Stanimirović, N. M. McClure-Griffiths +9

We present the first detection of HCO absorption in the Magellanic System. Using the Australia Telescope Compact Array (ATCA), we observed 9 extragalactic radio continuum sourc…

astro-ph.GA2014★ 101 cited

[CII] absorption and emission in the diffuse interstellar medium across the Galactic Plane

M. Gerin, M. Ruaud, J. R. Goicoechea +10

Ionized carbon is the main gas-phase reservoir of carbon in the neutral diffuse interstellar medium and its 158 micron fine structure transition [CII] is the most important cooling…

astro-ph.GA2009★ 20 cited

Imaging galactic diffuse clouds: CO emission, reddening and turbulent flow in the gas around Zeta Oph

H. S. Liszt, J. Pety, K. Tachihara

Methods: 12CO emission is imaged in position and position-velocity space analyzed statistically, and then compared with maps of total reddening and with models of the C+ - CO trans…

astro-ph2001★ 145 cited

The Spin Temperature of Warm Interstellar H I

H. Liszt

Collisional excitation of the 21cm HI hyperfine transition is not strong enough to thermalize it in warm neutral (``intercloud'') interstellar gas, which we show by simultaneously…