One-sided jet at milliarcsecond scales in LS I +61˚ 303

We present Very Long Baseline Interferometry (VLBI) observations of the high mass X-ray binary LS I +61˚303, carried out with the European VLBI Network (EVN). Over the 11 hour observing run, performed ~10 days after a radio outburst, the radio source showed a constant flux density, which allowed sensitive imaging of the emission distribution. The structure in the map shows a clear extension to the southeast. Comparing our data with previous VLBI observations we interpret the extension as a collimated radio jet as found in several other X-ray binaries. Assuming that the structure is the result of an expansion that started at the onset of the outburst, we derive an apparent expansion velocity of 0:003 c, which, in the context of Doppler boosting, corresponds to an intrinsic velocity of at least 0:4 c for an ejection close to the line of sight. From the apparent velocity in all available epochs we are able to establish variations in the ejection angle which imply a precessing accretion disk. Finally we point out that LS I +61˚303, like SS 433 and Cygnus X-1, shows evidence for an emission region almost orthogonal to the relativistic jet

Hints for a fast precessing relativistic radio jet in LS I + 61° 303

Here we discuss two consecutive MERLIN observations of the X-ray binary LS I +61° 303 . The first observation shows a double-sided jet extending up to about 200 AU on both sides of a central source. The jet shows a bent S-shaped structure similar to the one displayed by the well-known precessing jet of SS 433 . The precession suggested in the first MERLIN image becomes evident in the second one, showing a one-sided bent jet significantly rotated with respect to the jet of the day before. We conclude that the derived precession of the relativistic (beta=0.6) jet explains puzzling previous VLBI results. Moreover, the fact that the precession is fast could be the explanation of the never understood short term (days) variability of the associated gamma-ray source 2CG 135+01 / 3EG J0241+6103

I-SS: integrated supervision systems approach based on interactive components

Process supervision is the activity focused on monitoring the process operation in order to deduce conditions to maintain the normality including when faults are present Depending on the number/distribution/heterogeneity of variables, behaviour situations, sub-processes, etc. from processes, human operators and engineers do not easily manipulate the information. This leads to the necessity of automation of supervision activities. Nevertheless, the difficulty to deal with the information complicates the design and development of software applications. We present an approach called "integrated supervision systems". It proposes multiple supervisors coordination to supervise multiple sub-processes whose interactions permit one to supervise the global process

Els precedents de la Catedral de Santa Maria de Girona. De la plaça religiosa del fòrum romà al conjunt arquitectònic de la seu romànica (ss. I aC - XIV dC)

S'estudia els precedents de l'actual edifici de la Catedral de Girona prenent com a guia bàsica les restes físiques detectades en el sector, combinant-les amb nombroses notícies procedents de la documentació escrita i la consideració de paral·lels. Un apartat historiogràfic posa de relleu les diferents opinions sobre la història de la Catedral i dels seus edificis d'ençà del segle XVII. El conjunt d'època romana consistia en la plaça religiosa del fòrum de la ciutat. Com que els segles de l'Antiguitat Tardana i Alta Edat Mitjana no deixaren rastre físic identificable, el següent conjunt arquitectònic estudiat és el de la catedral del segle XI (iniciada vers 1010), detallada en cadascuna de les seves parts així com en els seus aspectes generals (implantació, tècnica constructiva, decoració). Finalment, l'estudi del conjunt claustral (configuració i funcions) permet aclarir determinats aspectes de la història institucional del capítol de la Catedral.