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On the infrared void in the Lupus dark clouds
Strömgren uvbyβ photometry observations obtained for 205 starsin the general direction of a void in the IRAS 100-μm emission fromthe Lupus dark cloud complex are presented and analysed. The colourexcess versus distance diagram confirms the existence of a regiondepleted from interstellar material, which is also seen in the ROSATsoft X-ray background emission map. The distance to the surroundingmaterial is estimated as being within the interval from 60 to 100pc.This result is in disagreement with previous distance estimates to thesupposed supernova that has been suggested as responsible for clearingthe region from dust. As an alternative, the data presented support thesuggestion that the void may have been produced by the detachment ofmaterial from the interface between LoopI and the Local Bubble as aconsequence of hydromagnetic instabilities. Moreover, the distributionof colour excess as a function of distance supports a value of ~150pc asthe most probable distance to the dark cloud known as Lupus1.
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Membro dei seguenti gruppi:
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Osservazione e dati astrometrici
| Costellazione: | Lupo |
| Ascensione retta: | 15h26m02.26s |
| Declinazione: | -30°06'14.8" |
| Magnitudine apparente: | 9.723 |
| Moto proprio RA: | 13.2 |
| Moto proprio Dec: | -11.6 |
| B-T magnitude: | 10.613 |
| V-T magnitude: | 9.797 |
Cataloghi e designazioni:
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