By Marilyn Singer

Contributor note: Illustrated via Meilo So
Publish yr note: First released in 2002
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This provocative selection of poems levels from such lofty matters as an astronaut’s view of Earth to the burrows of worms and little creatures in the earth, “where i attempt to tread softly: a quiet mammoth leaving basically footprints at the roof.”

Marilyn Singer’s lilting unfastened verse bargains visible pictures that supply us clean new insights and recognize for the strong energy of volcanoes, fens, islands, deserts, dunes, and traditional failures. Singer’s simply available poems additionally comprise the various lighter moments of adolescence, comparable to sliding on ice and taking part in in dust. Meilo So’s detailed india ink drawings on rice paper supply an extremely good-looking show off for those buoyant nature poems.

From the Hardcover edition.

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371-381. : 1950, Publ. Astron. Soc. 14-15. : 1973, Astrophys. J. 229-237. IR PHOTO~~TRY OF SYMBIOTIC STARS AT CALAR ALTO OBSERVATORY C. Eiroa, H. 2 m telev scope of the Calar Alto Observatory on July 1981, and are reported in the figure. Three stars (Z And, CI Cyg, V1329 -11 Cyg) were observed during a phase V1Ol6Cyg of minimum activity. 55 to 5 u energy spectrum, which is a! CICyg tributed to the late type star with -12 a colour temperature close to 3000K. 67 u to 5 u, where the cool spectrum dominates, while shortwards -13 there is a large contribution of the "nebular" component, which increased during the recent outburst.

Astron. Union. Colloq. 125-149. : 1980a, Monthly Notices Roy. Astron. Soc. 521-530. : 1980b, Astrophys. 131-133. : 1981, Proc. N. Amer. Workshop Symbiotic Stars, in press. : 1978, Monthly Notices Roy. Astron. Soc. 57P-60P. : 1974, Monthly Notices Roy. Astron. Soc. 337-350. : 1975, Monthly Notices Roy. Astron. Soc. 579-587. : 1976, Astron. Astrophys. 119-121. : 1979, Monthly Notices Roy. Astron. Soc. 813-816. : 1981, Proc. N. Amer. Workshop Symbiotic Stars, in press. : 1970, Chapter 3 in "Eruptive Stars", Eds.

The giant sequence is represented by the irregular curve. Crosses indicate D-type systems. If the dust were the dominant emission mechanism, the data should fallon the black-body line, which is marked with temperatures in Kelvin. Combinations of cool star and dust map out a range of locations on the diagram; the combination of an M5 giant with a 1000K dust shell is shown. The four D-type stars near the foot of the diagram must have cool components hotter than 5000K. The Magellanic Cloud symbiotic stars are included in this group.

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