Dark molecular gas in Pegasus–Pisces

We examine the molecular content of a large region (∼2200 square degrees) in Pegasus–Pisces with an estimated dark molecular gas fraction of 59 per cent. Using the extensive CO(1-0) Southern Galactic hemisphere, high-latitude survey by Magnani et al. (2000), we re-examined the CO-detectable mass est...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2019-06, Vol.486 (2), p.2281-2289
Hauptverfasser:	Donate, Emmanuel, Blair, Samantha, Chilton, Zachary, Gladney, Codie, Gordon, Jeremy W, Goulart, Micah C, Magnani, Loris
Format:	Artikel
Sprache:	eng
Online-Zugang:	Volltext
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