"De Mayrit al cielo": a mass function from 18 to 0.003 Msol in sigma Orionis

Details "De Mayrit al cielo": a mass function from 18 to 0.003 Msol in sigma Orionis "De Mayrit al cielo": a mass function from 18 to 0.003 Msol in sigma Orionis

Nov 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011hsa6.conf..527c&link_type=abstract

Highlights of Spanish Astrophysics VI, Proceedings of the IX Scientific Meeting of the Spanish Astronomical Society (SEA), held

Astronomy and Astrophysics

Astrophysics

Scientific paper

The star sigma Orionis A (O9.5 V) is visible with the naked eye, illuminates the mane of the Horsehead Nebula and, with about 18 Mdol, is the most massive one in the homonymous cluster. S Ori 70 (T6) is, with about 0.003 Msol, the least massive isolated body yet found outside of the Solar System. Covering the whole mass interval in between, the sigma Orionis cluster has Herbig Ae/Be and T Tauri stars, proplyds, X-ray emitters, Herbig-Haro objects, variable brown dwarfs, ``isolated planets''... The Mayrit catalogue is the result of a continuous effort to study in depth one of the most important star-forming regions.

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