other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
1999MNRAS.302..417S - Mon. Not. R. Astron. Soc., 302, 417-436 (1999/January-3)
The large-scale H I structure of the Small Magellanic Cloud.
STANIMIROVIC S., STAVELEY-SMITH L., DICKEY J.M., SAULT R.J. and SNOWDEN S.L.
Abstract (from CDS):
A kinematic study of the HI data reveals the existence of three supergiant shells which were previously undetectable in the ATCA data alone. These shells have diameters up to 1.8 kpc and require energies (in the standard supernova-driven models) up to 2x1054 erg. The structure and evolution of the ISM in the SMC are heavily influenced by the formation of these supergiant shells.
Abstract Copyright: 1998, Royal Astronomical Society
Journal keyword(s): turbulence - ISM: clouds - ISM: structure - galaxies: individual: Small Magellanic Cloud - Magellanic Clouds - galaxies: structure
Nomenclature: Table 2: [SSD99] SGS NNNA (Nos 37A, 304A, 494A).
Simbad objects: 18
To bookmark this query, right click on this link: simbad:1999MNRAS.302..417S and select 'bookmark this link' or equivalent in the popup menu