HD 192281 and HD 10125: A Study of their Local ISM using Radio and Infrared Data

Details HD 192281 and HD 10125: A Study of their Local ISM using Radio and Infrared Data HD 192281 and HD 10125: A Study of their Local ISM using Radio and Infrared Data

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..15..200a&link_type=abstract

Winds, Bubbles, and Explosions: a conference to honor John Dyson, Pátzcuaro, Michoacán, México, September 9-13, 2002 (Eds. S. J.

Astronomy and Astrophysics

Astronomy

Ism: Bubbles, Radio Lines: Ism, Stars: Individual ( Hd 192281, Hd 10125)

Scientific paper

Massive stars like HD 192281 (O5 V n((f))p) and HD 10125 (O9 5 Ib or
O9.7 II) have a substantial impact on their surrounding interstellar
medium (ISM) via their high Lyman continuum flux and their strong
stellar winds.

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