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Can the ballistic particle model explain the Hubble sequence?BASH, F; LEISAWITZ, D.The Astrophysical journal. 1984, Vol 285, Num 1, pp 25-43, issn 0004-637X, part 1Article

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Isotopic fractionation and mass motion in giant molecular cloudsPENZIAS, A. A.The Astrophysical journal. 1983, Vol 273, Num 1, pp 195-201, issn 0004-637XArticle

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CAN GIANT MOLECULAR CLOUDS FORM IN SPIRAL ARMS.CASOLI F; COMBES F.1982; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1982; VOL. 110; NO 2; PP. 287-294; BIBL. 36 REF.Article

Giant molecular clouds on M31. I. Molecular cloud propertiesROSOLOWSKY, E.The Astrophysical journal. 2007, Vol 654, Num 1, pp 240-251, issn 0004-637X, 12 p., 1Article

Giant molecular clouds are more concentrated toward spiral arms than smaller cloudsSTARK, Antony A; LEE, Youngung.The Astrophysical journal. 2006, Vol 641, Num 2, issn 0004-637X, L113-L116, 2Article