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Fig. 1

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Spectra of the observed transitions towards Haro 6-10. Top panel: 13CO J = 2−1 spectrum. Bottom panels, from top to bottom: spectra of 13CO J = 2−1, C17O J = 2−1, CN N = 2−1, ortho H2CO 313 − 212, ortho H2CO 312 − 211, and SO 54 − 43 presented on a common scale. The Y axis scale is antenna temperature, (the conversion factor to flux density is 9 Jy/K).

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