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Star Formation in the Vela Molecular Clouds: H2 Imaging Survey

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The Impact of Large Scale Near-IR Sky Surveys

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 210))

Abstract

In the framework of an observational study of the young stellar content in the Vela star forming clouds, we are currently carrying out broad- and narrow-band imaging (K and H2 at 2.122 μm) of a complete IRAS selected sample of Young Stellar Objects (YSOs). Here we present the results for the source IRAS 08448–4343 which reveals H2 emission aligned in a bipolar and well collimated jet.

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References

  • Giannini, T. et al. 1996 in Proc. ESO Workshop on the Role of Dust in the Formation of Stars, in press

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  • Liseau, R., Lorenzetti, D., Nisini, B., Spinoglio, L., & Moneti, A. 1992, A&A, 265, 577

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  • Lorenzetti, D., Spinoglio, L., & Liseau, R. 1993, A&A, 275, 489

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© 1997 Springer Science+Business Media Dordrecht

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Lorenzetti, D., Massi, F., Scaramella, R., Vitali, F., Giannini, T. (1997). Star Formation in the Vela Molecular Clouds: H2 Imaging Survey. In: Garzón, F., Epchtein, N., Omont, A., Burton, B., Persi, P. (eds) The Impact of Large Scale Near-IR Sky Surveys. Astrophysics and Space Science Library, vol 210. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5784-1_31

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  • DOI: https://doi.org/10.1007/978-94-011-5784-1_31

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-6442-2

  • Online ISBN: 978-94-011-5784-1

  • eBook Packages: Springer Book Archive

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