Star Formation Around the Supernova Remnant G24.7+0.6

Petriella A.; Paron S.; Giacani E.

Vol. 40 No. 1 (2011), Contributions

Vol. 40 No. 1 (2011)

Contributions

Star Formation Around the Supernova Remnant G24.7+0.6

Petriella A.⁺⁻
Paron S.⁺⁻
Giacani E.⁺⁻

Petriella A.

Instituto de Astronomía y Física del Espacio (IAFE, CONICET-UBA), CC 67, Suc. 28, 1428 Buenos Aires, Argentina

Paron S.

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Giacani E.

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Keywords

ISM: supernova remnants
ISM: clouds
stars: formation

How to Cite

Star Formation Around the Supernova Remnant G24.7+0.6. (2011). Revista Mexicana De Astrofísica Y Astronomía Serie De Conferencias, 40(1), 194-194. https://astronomia.unam.mx/journals/rmxac/article/view/2011rmxac..40..194p

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Abstract

We identify young stellar object candidates around the supernova remnant G24.7+0.6. They appear located in the molecular gas probably perturbed by the remnant. We suggest that G24.7+0.6 and its progenitor could have triggered the formation of new stars.

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Star Formation Around the Supernova Remnant G24.7+0.6

Keywords

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