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- W4238452357 abstract "IRAS Calibrated Raw Detector Data (CRDD) are presented of a part of the Cygnus-X region, incorporating W75, DR21 and W75N, and a previously unknown loop of dust emission is observed. This loop is interpreted as a spherical shell-like shock front, and two alternative explanations for its origin are explored — a wind-blown bubble around an OB association, and an old supernova remnant. The arguments for each are outlined, and it is deduced that there are insufficient OB stars old enough to have formed the loop by combined stellar wind action, although a SNR appears consistent with the data." @default.
- W4238452357 created "2022-05-12" @default.
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- W4238452357 date "1991-01-01" @default.
- W4238452357 modified "2023-10-17" @default.
- W4238452357 title "The W75 — Cygnus - X IRAS loop:- OB - ‘Bubble’ or SNR?" @default.
- W4238452357 cites W1983968731 @default.
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- W4238452357 doi "https://doi.org/10.1017/s0074180900199607" @default.
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