X-ray probing for protostars

Details X-ray probing for protostars X-ray probing for protostars

Feb 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002asthe..95...77t&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 95, No. 2, p. 77 - 83 (2002)

Other

Protostars, X Rays

Scientific paper

After long preparation of 20 years, Chandra X-ray Observatory was launched in July 1999. With two orders of magnitudes higher spatial resolution (FWHM 0.5") and two orders of magnitudes lower detection limit than those of the previous satellites, we now have a new tool to examine closest look yet at the youngest stars in the Universe, never before detected because they are hidden within dust and molecular clouds that filter all other types of light. Protostars with thick veils are now being unvailed.

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