The emission/reflection nature of Herbig-Haro object 24

Details The emission/reflection nature of Herbig-Haro object 24 The emission/reflection nature of Herbig-Haro object 24

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...234l.191s&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 234, Dec. 15, 1979, p. L191-L194.

Astronomy and Astrophysics

Astrophysics

37

Herbig-Haro Objects, Nebulae, Stellar Structure, Emission Spectra, Line Spectra, Stellar Evolution, Stellar Winds

Scientific paper

Observations of Herbig-Haro object 24 with a new spectropolarimeter confirm that the characteristic emission-line spectra of H-H objects are produced in situ. The outflowing wind which shock-heats the H-H 24 knots arises in a T Tauri-like star embedded in the associated dark cloud. This star is also the source of the H-H optical continuum, which becomes strongly polarized when scattered off dust in the knots.

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