The young open cluster Berkeley 55

We present UBV photometry of the highly reddened and poorly studied open cluster Berkeley 55, revealing an important population of B-type stars and several evolved stars of high luminosity. Intermediate-resolution far-red spectra of several candidate members confirm the presence of one F-type supergiant and six late supergiants or bright giants. The brightest blue stars are mid-B giants. Spectroscopic and photometric analyses indicate an age 50 ± 10 Myr. The cluster is located at a distance d ≈ 4 kpc, consistent with other tracers of the Perseus Arm in this direction. Berkeley 55 is thus a moderately young open cluster with a sizable population of candidate red (super)giant members, which can provide valuable information about the evolution of intermediate-mass stars.

Introducing more equity in the CAP: a difficult challenge. Egmont Paper #55, June 2012

[From the Introduction]. The main question addressed by this paper is how to reach a more equitable distribution of CAP’s payments pragmatically, politically and economically? Pragmatically, the CAP is a multi-functional policy, which has to combine different goals, i.e. to be more equitable, green and market-oriented. However, these objectives are not always compatible and require trade-offs. Politically, regarding the CAP’s significant share (40%) of the EU budget and the current public debt crisis, Member States are most likely to keep their attention on the juste retour calculations rather than the promotion of the European public interest in the EU negotiations. Economically, reaching a more equitable distribution of payments should be achieved without significant disruptive changes that could have serious consequences on the costs and benefits of the agricultural sector in the EU. Considering these elements, it is already clear that reaching a more equitable distribution of CAP’s payments represents a difficult challenge.