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Molecular gas and star formation towards the IR dust bubble S 24 and its environs
(EDP SCIENCES, 2015)
Aims. We present a multi-wavelength analysis of the infrared dust bubble S 24, and the extended IR sources G341.220-0.213 and
G341.217-0.237 located in its environs, with the aim of investigating the characteristics of ...
Interactions of the Infrared bubble N4 with ITS surroundings
(IOP Publishing, 2016-02)
The physical mechanisms that induce the transformation of a certain mass of gas in new stars are far from being well understood. Infrared bubbles associated with H ii regions have been considered to be good samples for ...
A submillimeter study of the IR dust bubble s 21 and its environs
(Universidad Nacional Autonoma de Mexico, 2017)
Based on the molecular emission in the 12CO(2-1) and 13CO(2-1) lines, and on the continuum emission in the MIR and FIR towards the S 21 IR dust bubble, we analyze the physical characteristics of the gas and dust linked to ...
COMPARISONS OF THE INTERSTELLAR MAGNETIC FIELD DIRECTIONS OBTAINED FROM THE IBEX RIBBON AND INTERSTELLAR POLARIZATIONS
(IOP PUBLISHING LTD, 2010)
Variations in the spatial configuration of the interstellar magnetic field (ISMF) near the Sun can be constrained by comparing the ISMF direction at the heliosphere found from the Interstellar Boundary Explorer (IBEX) ...
Hydrodynamical simulations of Galactic fountains - I. Evolution of single fountains
(WILEY-BLACKWELL, 2008)
The ejection of the gas out of the disc in late-type galaxies is related to star formation and is due mainly to Type II supernovae. In this paper, we studied in detail the development of the Galactic fountains in order to ...