Imaging studies of localized, ionized flows in the Rosette nebula

Details Imaging studies of localized, ionized flows in the Rosette nebula Imaging studies of localized, ionized flows in the Rosette nebula

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26a...334..264c&link_type=abstract

Astronomy and Astrophysics, v.334, p.264-268 (1998)

Astronomy and Astrophysics

Astrophysics

9

Ism: Individual Objects: Rosette Nebula, Ism: Jets And Outflows, H Ii Regions, Infrared: Ism: Lines And Bands

Scientific paper

Optical ([S ii] 6717 & 6731 Angstroms, [Siii] 9069 Angstroms}, [O iii] 5007 Angstroms and Hα + [N ii] 6584 Angstroms), K-band, H_2 1-0 S(1) 2.122mu m and [Fe ii] 1.64mu m imagery has been obtained of a group of high-speed knots close to the core of the Rosette nebula. A high-speed, high-excitation, bow-shaped structure has been directly imaged in [O iii] 5007 Angstroms for the first time and is interpreted as a bow shock either at the head of a collimated flow or around a fast-moving molecular bullet. Two candidates for the driving source of these motions have also been identified in a system where no sources were previously known.

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