Triggered star formation in a molecular shell created by a SNR?
We present a study of a new molecular shell, G 126.1-0.8-14, using available multiwavelength Galactic plane surveys and optical Gemini observations. A well-defined shell-like structure is observed in the CO(1-0) line emission at (l,b) = (126°.1, -0°.8), in the velocity range -10.5 to -15.5 kms-1. Th...
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2014
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00358711_v438_n2_p1089_Cichowolski http://hdl.handle.net/20.500.12110/paper_00358711_v438_n2_p1089_Cichowolski |
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