... The collision results in rapid heating (the socalled ``shock process"), so that the "shocked" regions start to shine in the light of various ionized elements; they are similar to the "Herbig-Haro" objects. ...
... The collision results in rapid heating (the socalled ``shock process"), so that the "shocked" regions start to shine in the light of various ionized elements; they are similar to the "Herbig-Haro" objects. ...
... The collision results in rapid heating (the socalled ``shock process"), so that the "shocked" regions start to shine in the light of various ionized elements; they are similar to the "Herbig-Haro" objects. ...
... The collision results in rapid heating (the socalled ``shock process"), so that the "shocked" regions start to shine in the light of various ionized elements; they are similar to the "Herbig-Haro" objects. ...
... In addition, observations of the Crab pulsar demonstrate a new observing mode, high-speed photometry. eso9948b shows a three-colour composite of the young objectHerbig-Haro 34 (HH-34) , now in the protostar stage of evolution. ...
... In addition, observations of the Crab pulsar demonstrate a new observing mode, high-speed photometry. eso9948b shows a three-colour composite of the young objectHerbig-Haro 34 (HH-34) , now in the protostar stage of evolution. ...