UVBY-Beta Photometry for 67 Stars in the Region of Alpha-Persei

UVBY-Beta photometric data are presented for 67 stars in the region of alpha-Persei and their relationship to the cluster is analyzed. These data allowed us to confirm at least 16 new members of the alpha-Persei open cluster.

UBVRI photometry of G, K, M Hipparcos stars. II.

As indicated by Grenon (1989), the data of the present series of reports on the UBVRI photometry of late-type stars in the Hipparcos Input Catalog are to be employed in computations of Hipparcos observing time, as well as in evaluating the observability of faint stars by the satellite. Attention is here given to late type stars in the V = 8-12 range, including distant red giants in the Galactic plane (Hipparcos proposal 189), as well as high proper motion stars included in the G, LTT, LP, and MCC catalogs.

A type stars - physical parameters from UVBY and H-beta photometry

uvby H-beta photometry has been obtained for a sample of 93 selected main sequence A stars. The purpose was to determine accurate effective temperatures, surface gravities, and absolute magnitudes for an individual determination of ages and parallaxes, which have to be included in a more extensive work analyzing the kinematic properties of A V stars. Several calibrations and methods to determine the above mentioned parameters have been reviewed, allowing the design of a new algorithm for their determination. The results obtained using this procedure were tested in a previous paper using uvby H-beta data from the Hauck and Mermilliod catalogue, and comparing the rusulting temperatures, surface gravities and absolute magnitudes with empirical determinations of these parameters.

Reliure de : Georgii Agricolae de Re metallica libri XII, quibus officia, instrumenta, machinae ac omnia... ad metallicam spectantia non modo... describuntur, sed et per effigies... ob oculos ponuntur... Ejusdem de animantibus subterraneis liber...

Numérisation partielle de reliure

Maximum mass of neutron stars

We determine the structure of neutron stars within a Brueckner-Hartree-Fock approach based on realistic nucleon-nucleon, nucleon-hyperon, and hyperon-hyperon interactions. Our results indicate rather low maximum masses below 1.4 solar masses. This feature is insensitive to the nucleonic part of the EOS due to a strong compensation mechanism caused by the appearance of hyperons and represents thus strong evidence for the presence of nonbaryonic "quark" matter in the interior of heavy stars.

La visión teofánica en el sufismo de Ibn al-'Arabî (ob. 638/1240)

Un conocido dicho sufí dice que: "El color del agua es el color de su recipiente". Para hablar de la visión teofánica, al-Junayd, Ibn 'Arabi y otros muchos místicos invocaban frecuentemente este símbolo. Según al-Bistami, el color del recipiente -el corazón del contemplador- da "color" al agua que en sí es invisible; según Ibn 'Arabi, no es el corazón quien da su "color" a la Forma que recibe, sino que, a la inversa, el corazón del gnóstico "se colorea" en cada instante con el color, es decir, con la modalidad de la Forma bajo la cual el Ser divino se epifaniza en él. Así es como "l gnóstico,asume las peculiaridades del carácter de Dios, hasta tal punto que parece como si él fuera El". El propósito del presente artículo es analizar la teoría neoplatónica de la manifestación de lo divino expresada por medio de dos parábolas -el color del agua y el color del vidrio- presentes tanto en la tradición islámica como en la judía.

LS 5039: A runaway microquasar ejected from the galactic plane

We have compiled optical and radio astrometric data of the microquasar LS 5039 and derived its proper motion. This, together with the distance and radial velocity of the system, allows us to state that this source is escaping from its own regional standard of rest, with a total systemic velocity of about 150 km/s and a component perpendicular to the galactic plane larger than 100 km/s. This is probably the result of an acceleration obtained during the supernova event that created the compact object in this binary system. We have computed the trajectory of LS 5039 in the past, and searched for OB associations and supernova remnants in its path. In particular, we have studied the possible association between LS 5039 and the supernova remnant G016.8-01.1, which, despite our efforts, remains dubious. We have also discovered and studied an HI cavity in the ISM, which could have been created by the stellar wind of LS 5039 or by the progenitor of the compact object in the system. Finally, in the symmetric supernova explosion scenario, we estimate that at least 17 solar masses were lost in order to produce the high eccentricity observed. Such a mass loss could also explain the observed runaway velocity of the microquasar.

Stars and Strings für Jazzensemble u. Streichorchester

Soitinnus: jazzyhtye, jousiorkesteri.

Nova mappa geographica Sueciae ac Gothiae regna ut et Finlandiae ducatum ac Lapponiam, cum provinciis minoribus, ob oculos ponens, cura et sumtibus Tobiae Conradi Lotter, chalcogr et geogr: Augustae Vindel.

Alareunassa privilegiomerkintä: Cum gratia et privil. s. r. i. vicariatq, in partibq Rheni, Sveviae, et juris Franconici.