Spontaneous and Induced Star Formation in the LMC

dc.creatorEfremov, Y. N.
dc.creatorElmegreen, B. G.
dc.date1998-11-13
dc.date.accessioned2026-07-07T02:29:06Z
dc.date.available2026-07-07T02:29:06Z
dc.descriptionSpontaneous and triggered star formation in the LMC is discussed with data on star clusters ages and positions. The supershell LMC4 and the stellar arcs in the same region are suggested to be triggered by GRBs, the progenitors of which might have escaped the old elliptical cluster NGC1978, close to which are a number of X-ray binaries and the SGR/SNR N49.
dc.description5 pages, 0 figures, IAU Symposium 190, "New Views of the Magellanic Clouds," ASP Conference Series, eds. Yuo-Hua Chu et al., 1999. (A conference held in Victoria, British Columbia, Canada, 12 - 17 July 1998.)
dc.identifierhttps://arxiv.org/abs/astro-ph/9811216
dc.identifierhttp://arxiv.org/abs/astro-ph/9811216
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13337
dc.subjectAstrophysics
dc.titleSpontaneous and Induced Star Formation in the LMC
dc.typetext

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