Fig. 3
Herschel dust temperature map of the Ophiuchus molecular cloud at a HPBW resolution of 36.3′′. The dust temperature was derived by SED fitting from 160 to 500 μm. The warmest regions are located around S1, east of Oph A, and HD 147889, while the warm shell to the northwest is driven by the star ρ Ophiuchi. These three objects are B-type stars, S1 and HD 147889 being both young members of the L1688 infrared star cluster.
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