ar X iv : 0 70 6 . 18 56 v 2 [ as tr o - ph ] 1 4 A ug 2 00 7 Solar transition region features observed with Hinode / EIS

ar X iv : 0 70 6 . 18 57 v 2 [ as tr o - ph ] 1 4 A ug 2 00 7 EUV emission lines and diagnostics observed with Hinode / EIS

P. R. Young, G. Del Zanna, H. E. Mason, K. P. Dere, E. Landi, M. Landini, G. A. Doschek, 1STFC Rutherford Appleton Laboratory, Chilton, Didcot, Oxfor 2University College London, Department of Space and Climate Physics, 3DAMTP, Centre for Mathematical Sciences, 4George Mason University, 4400 University Dr., Fairfax 5Artep, Inc at Naval Research Laboratory, 4555 Overlook Ave. S.W., 6Dipartimento ...

ar X iv : 0 70 8 . 26 18 v 1 [ as tr o - ph ] 2 0 A ug 2 00 7 Using Local Volume data to constrain Dark Matter dynamics

ar X iv : 0 70 5 . 31 41 v 1 [ as tr o - ph ] 2 2 M ay 2 00 7 The SARG Planet Search

ar X iv : 0 80 7 . 35 56 v 2 [ as tr o - ph ] 2 7 A ug 2 00 8 Astrophysical relevance of γ transition energies

The relevant γ energy range is explicitly identified where additional γ strength has to be located for having an impact on astrophysically relevant reactions. It is shown that folding the energy dependences of the transmission coefficients and the level density leads to maximal contributions for γ energies of 2 ≤ Eγ ≤ 4 unless quantum selection rules allow isolated states to contribute. Under t...

ar X iv : 0 70 8 . 38 56 v 1 [ as tr o - ph ] 2 8 A ug 2 00 7 Young Star Clusters in M 31

In our study of M31’s globular cluster system with MMT/Hectospec, we have obtained high-quality spectra of 85 clusters with ages less than 1 Gyr. With the exception of Hubble V, the young cluster in NGC 205, we find that these young clusters have kinematics and spatial distribution consistent with membership in M31’s young disk. Preliminary estimates of the cluster masses and structural paramet...