Nova 1998 2 in M31 this image of the second Nova in M31 in 1998, was made from 38 exposures of 45 seconds integration time. It was made at September 21, 22h 20m UT. Telescope was a CG11 at f/6.3, no filters were used. The long list of processing steps caused the artefacts at the overexposed center of the galaxy and in many of the brighter stars. During the exposures thin clouds covered the sky but the CCD cuts through them, allowing me to obtain this result. ...

... C'est d'abord un numГїro d'immatriculation : 2008 TC3. Un caillou parmi des milliards d'autres, comme il arrive Г la Terre d'en croiser rГїguliГЕrement dans sa course autour du Soleil. ... Trop petit pour le ranger dans la classe des astГїroГ?des ; trop gros pour le voir comme une Гїtoile filante au moment oГ? il entre en collision avec notre planГЕte. ... Savoir pour prГїvoir et, dans le futur, pour les gros objets, imaginer comment s'en prГїmunir n'est plus de la science-fiction. ...

... Maps of six sources (0420+022, 0420-014, 1308+326, 1345+125, 1803+784, and DA 193) obtained with milliarcsecond resolution are presented and discussed, together with their broadband (1­22 GHz) spectra obtained on the RATAN­600 radio telescope at epochs close to those of the VLBI observations. ... The image (Fig. 5) shows that the source structure at 18 cm is compact, consisting of a VLBI core and two jet components, with the outer component lying 5 mas (30 pc) to the northwest of the core ( = 54 ). ...

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