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Depth structure in the gas in Shapley III along three lines of sight
1991
Symposium - International astronomical union
Shapley Constellation III in the Large Magellanic Cloud (LMC) is surrounded by a ring of HII regions, called Supershell LMC 4 (Meaburn 1980). In the direction of the centre of this spatial strucutre very little neutral interstellar gas is found (McGee & Milton 1964). The spatial arrangement suggests that a hole exists in the gas layer of the LMC, one which may be blown out by the effect of the winds of the stars of Constellation III or by supernova blasts from the same area. Shock waves
doi:10.1017/s0074180900201101
fatcat:mnjh6bt3ozdlratjwnql247gxe