We report high-resolution millimeter mapping with the IRAM Plateau de Bure interferometer of rest-frame 335μm continuum and CO(3–2) line emission from the z = 2.8 submillimeter galaxy SMMJ02399-0136. The continuum emission comes from a ∼ 3 diameter structure whose elongation is approximately east-west and whose centroid is coincident within the astrometric errors with the brightest X-ray and re...

We present a study of the density structure of the protostellar collapse candidate B335 using continuum observations from the IRAM Plateau de Bure Interferometer made at wavelengths of 1.2 mm and 3.0 mm. We analyze these data, which probe spatial scales from 5000 AU to 500 AU, directly in the visibility domain by comparison to synthetic observations constructed from models that assume different...

Geological settings are of major importance in selecting appropriate environment for disposal high-level radioactive waste from nuclear power plants. Clay rocks preferred a number countries as suitable host due to their insulating properties and ability self- seal cracks other disturbances. In Bulgaria, on the basis multi-criterion comparative analysis, several prospective sites have been selec...

Recently papers investigating problems on detection of the moment of occurrence of an attack on various systems were published. In particular, they consider ”Dos-attacks” or attacks like of ”denial of service” in a computing system and subsequent changes of the protocol of processing of input assignments. These studies are actual now. The main difference between the paper and previous works is ...

We present images of the Vega system obtained with the IRAM Plateau de Bure interferometer at 1.3 millimeters wavelength with sub-mJy sensitivity and ∼ 2. ′′ 5 resolution (about 20 AU). These observations clearly detect the stellar photosphere and two dust emission peaks offset from the star by 9. ′′ 5 and 8. ′′ 0 to the northeast and southwest, respectively. These offset emission peaks are con...

We report IRAM Plateau de Bure, millimeter interferometry of three z ∼2.4 to 3.4, SCUBA deep field galaxies. Our CO line observations confirm the rest-frame UV/optical redshifts, thus more than doubling the number of confirmed, published redshifts of the faint submillimeter population and proving their high-z nature. In all three sources our measurements of the intrinsic gas and dynami-cal mass...

We have carried out a high-sensitivity search for circumstellar disks around Herbig Be stars in the continuum at 1.4mm and 2.7mm using the IRAM interferometer at the Plateau de Bure (PdBI) . In this letter, we report data on three well studied B0 stars, MWC 1080, MWC 137 and R Mon. The two latter have also been observed in the continuum at 0.7 cm and 1.3 cm using the NRAO Very Large Array (VLA)...

Velebitsko je podgorje klimatski specifičan dio Jadranskoga mora s najjačim udarima bure. Cilj rada analizirati neke od glavnih klimatskih elemenata i indeksa na području Velebitskoga podgorja. Analizirani su podaci triju meteoroloških postaja: Senj sjevernom dijelu, zatim Jablanac te Karlobag koji smješteni središnjem dijelu Prema Köppenu klima u Velebitskom podgorju umjereno topla kišna klima...

Aims. The earliest phases of massive star formation in clusters are still poorly understood. Here, we test the hypothesis for high-mass star formation proposed in our earlier paper (Peretto et al. 2006) stating that a massive, ultra-dense core may be currently forming at the center of the collapsing NGC 2264-C protocluster via the gravitational coalescence of several intermediate-mass Class 0 o...