[YOM2003] HLCG 92-35 , the SIMBAD biblio

[YOM2003] HLCG 92-35 , the SIMBAD biblio (6 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST09:27:47


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Title First 3 Authors
2003ApJ...592..217Y 12 17 High-latitude molecular clouds in an H I filament toward the MBM 53, 54, and 55 complex: existence of an H2Cloud with low CO intensity. YAMAMOTO H., ONISHI T., MIZUNO A., et al.
2006ApJ...642..307Y 16 11 Large-scale CO observations of a far-infrared loop in Pegasus: detection of a large number of very small molecular clouds possibly formed via shocks. YAMAMOTO H., KAWAMURA A., TACHIHARA K., et al.
2014ApJ...796...59F 371 T K A     X         9 24 43 HI, CO, and Planck/IRAS dust properties in the high latitude cloud complex, MBM 53, 54, 55 and
HLCG 92-35. Possible evidence for an optically thick HI envelope around the CO clouds.
FUKUI Y., OKAMOTO R., KAJI R., et al.
2015ApJ...798....6F 79           X         2 40 82 Optically thick H I dominant in the local interstellar medium: an alternative interpretation to "dark gas". FUKUI Y., TORII K., ONISHI T., et al.
2016MNRAS.460L..10B 83           X         2 5 46 Resolving the planetesimal belt of HR 8799 with ALMA. BOOTH M., JORDAN A., CASASSUS S., et al.
2017ApJ...838..132O 199           X C       4 26 22 H I, CO, and dust in the Perseus cloud. OKAMOTO R., YAMAMOTO H., TACHIHARA K., et al.

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