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245 10 $a GS263-02+45 : $b a new HI supershell with evidence of having triggered star formation? / $c E. Marcelo Arnal, Mariela Corti.
490 0# $a Trabajos publicados del IAR ; $v no. 798
520 ## $a Aims: we look for the galactic neutral hydrogen (HI) supershells likely to be associated with massive star groupings. Methods: a neutral hydrogen (HI) linesurvey carried out at the Instituto Argentino de Radioastronomía (IAR) and the Southern Galactic Plane Survey (SGPS) were the main databases used in this investigation. Results: a new HI supershell (G263-02+45) was found in the outer part of the Galaxy. This structure is located at a distance of 5.3 ñ 1 kpc from the Sun and has a linear diameter of about 665 ñ 40 pc. The expantion velocity of the supershell is ~ 14 km s. 1. The total amount of atomic gas related to GS263-02+45 is ~ 2X10. M. Based on the analysis of the SGPS HI data it concluded that the OB-association Bochum 7 is likely to be interacting with GS263-02+45. This fact together with distance and age arguments may indicate that Bochum 7 was born as a consequence of the evolution of GS263-02+45.
773 0# $7 ||as $t Astronomy and astrophysics. $d París : EDP Sciences. $g Vol. 476, no. 1, (2007), p. 255-261. $x 0004-6361
100 1# $a Arnal, E. M. $q (Edmundo Marcelo)
700 1# $a Corti, M. A. $q (Mariela A.)
653 ## $a Kinematics.
653 ## $a Dynamics.
653 ## $a Galaxy.
653 ## $a ISM.
653 ## $a Interstellar bubbles.
653 ## $a Radio lines.
653 ## $a Neutral hydrogen.
040 ## $a AR-BaBIR $b spa
856 ## $u http://adsabs.harvard.edu/abs/2007A%26A...476..255A $y ADS

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