Observational evidence for supernova-induced star formation - Canis Major R1

Astronomy and Astrophysics – Astronomy

Scientific paper

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Early Stars, Nebulae, Star Formation, Supernova Remnants, Astronomical Maps, Astronomical Photography, Hydrogen Clouds, Protostars, Ring Structures, Sky Surveys (Astronomy), Stellar Models

Scientific paper

Observational evidence is presented which indicates that star formation in the young association CMa R1 was initiated by a supernova explosion (probably of Type II) that occurred about half a million years ago. Palomar Sky Survey prints, neutral-hydrogen maps, and radial-velocity data are examined which show that the CMa R1 association is located on the outer edge of a ring of optical and radio emission, that an expanding neutral-hydrogen shell is coincident with the optical feature, and that HD 54662 is a runaway star in the CMa OB1 association and may be associated with the event that produced the observed supernova remnant. The optical and radio features are interpreted as a supernova remnant with an age of about 500,000 years and an initial outburst energy of the order of 5 by 10 to the 50th power ergs, which is expanding into an initially nonuniform medium characterized by an initial atomic-hydrogen density of approximately 1 per cu cm in the direction toward CMa R1 and less than half that value in the direction toward the sun.

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