Survey of Class 0 Protostars in the Smallest Clouds "Bok Globules"

Details Survey of Class 0 Protostars in the Smallest Clouds "Bok Globules" Survey of Class 0 Protostars in the Smallest Clouds "Bok Globules"

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009xmm..prop...27t&link_type=abstract

XMM-Newton Proposal ID #06509103

Computer Science

Stars, White Dwarfs, Solar System, Fest1-457, Cb68, Cb244

Scientific paper

We propose a survey of five nearby Bok globules to search for X-rays from Class 0 protostars. X-rays from Young Stellar Objects are likely to originate from the near vicinity of the star itself. The detection of the X-rays from Class 0 protostars, therefore, is of particular importance, providing direct evidence that the central star has been born. However, the protostars are usually deeply embedded within the cloud, so that, even the X-rays were completely absorbed. Bok globules are known as star formation sites surrounded by light and small molecular clouds of 10 Mo. The small absorption column of Bok globules gives us an opportunity to search whether X-rays "turn-on" occurs during the Class 0 phase and if so, when?

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