On the contributions of the Orion reflection nebulosity to the continuous UV spectrum of the Herbig-Haro objects HH 1 and HH 2 and of the C-S Star

Details On the contributions of the Orion reflection nebulosity to the continuous UV spectrum of the Herbig-Haro objects HH 1 and HH 2 and of the C-S Star On the contributions of the Orion reflection nebulosity to the continuous UV spectrum of the Herbig-Haro objects HH 1 and HH 2 and of the C-S Star

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...270l..59m&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 270, July 15, 1983, p. L59-L61.

Astronomy and Astrophysics

Astrophysics

11

Cn Emission, Continuous Spectra, Emission Spectra, Herbig-Haro Objects, Orion Nebula, Reflection Nebulae, Ultraviolet Spectra, Iue, Line Spectra, Radiant Flux Density, Stellar Spectra

Scientific paper

The possibility of contamination of the published UV continuum spectra of the Herbig-Haro objects HH 1 and HH 2 and the Cohen-Schwartz (C-S) star by the Orion reflection nebulosity (ORN) is pointed out. OAO 2 data suggest that the UV continuum observed in the environment of the C-S star may possibly be accounted for by the emission from the ORN. In the case of HH 1 and HH 2, the data suggest that there could be a contamination of the published spectra at λ ≤ 1500 Å of the order of 30%-50%.

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