1,481 research outputs found
Ukulele Lady
Get PDF[Verse 1]I saw the splendour of the moonlight On Honolulu BayThere’s something tender in the moonlight, On Honolulu Bay; And all the beachers Are fill of peachersWho brings their “ukes” along,And in the glimmer of the moonlight They love to sing their song.
[Verse 2] She used to sing to me by moonlight, On Honolulu Bay, Dond mem’ries cling to me by moonlight,Altho’ I’m far away. Someday I’m going Where eyes are glowingAnd lips are made to kiss, To see somebody in the moonlightAnd hear the song I miss.
[Chorus]If you like a Ukulele Lady like a you.If you like to longer where its shady, Ukulele Lady linger too. If you kiss a Ukulele Lady, Will you promise ever to be true? And she see another Ukulele Lady around with you Maybe she’ll sigh, Maybe she’ll cry, Maybe she’ll find somebody else, By and by to sing to, When it’s cool and shady, Where the tricky Wicki Wackies won;If you like a Ukulele Lady, Ukulele Lady like a you
On Membership, Humility, and Pedagogical Responsibilities: A Correspondence on the Work of Wendell Berry
Get PDFWendell Berry is a novelist, essayist, conservation activist and farmer who has had a lot to say over the last half century about the impact of modern industrial society on small farm communities and the land especially since WWII. In this three-way conversation, the authors take up central aspects of Berry’s work to think about how it has influenced their thinking as teacher educators focused on the intersections between social and ecological crises challenging our world. Themes of responsibility, leadership, community membership, friendship, “settler colonialism,” racism, land use, and ecological sustainability are brought to bear on education for just and healthy communities
Where the Water Lilies Grow
Get PDFhttps://digitalcommons.library.umaine.edu/mmb-vp/3761/thumbnail.jp
How Protostellar Outflows Help Massive Stars Form
Full text linkWe consider the effects of an outflow on radiation escaping from the
infalling envelope around a massive protostar. Using numerical radiative
transfer calculations, we show that outflows with properties comparable to
those observed around massive stars lead to significant anisotropy in the
stellar radiation field, which greatly reduces the radiation pressure
experienced by gas in the infalling envelope. This means that radiation
pressure is a much less significant barrier to massive star formation than has
previously been thought.Comment: 4 pages, 2 figures, emulateapj, accepted for publication in ApJ
Letter
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