[PDF] Top 20 Supersoft X rays nebulae in the Large Magellanic Cloud
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Supersoft X rays nebulae in the Large Magellanic Cloud
... this: the time-averaged luminosity of the SSSs is lower than the luminosity inferred from current X-rays observations, or the supersoft nebulae surface brightness ... See full document
206
The Proper Motion of the Large Magellanic Cloud Revisited
... for the QSO fields in ...represent the (X, Y ) positions of the QSO on different CCD frames, relative to the barycenter of the ...for the QSO in each CCD ... See full document
12
Radio Sources Embedded in the Dense Core B59, the “Mouthpiece” of the Pipe Nebula
... Very Large Array continuum observations made at 8.3 GHz toward the dense core B59, in the Pipe ...with the five most luminous sources at 70 µm in the region, while ... See full document
5
Planetary nebulae and the chemical evolution of the Magellanic Clouds
... that the IAG data do not include Ne abundances for the LMC, and that Stasi´ nska et ...galaxies. The sulfur abundances seem to be less reliable, as can be seen from the large stan- dard ... See full document
11
Properties of RR Lyrae stars in the inner regions of the Large Magellanic Cloud III Near infrared study
... For the ISPI ob- servations the observing strategy included alternating between the object and a nearby ...both the “object” and the “sky” pointings, we jittered within ∼20 arcsec to ... See full document
10
C130612a
... automating the reading process […] has thrown one style of picture analysis out of the world of images and into that of logical counts by electronic ... See full document
35
The Araucaria Project: an accurate distance to the late type double lined eclipsing binary ogle smc113 3 4007 in the small magellanic cloud
... with the WD code is presented in Figures 2 and ...with the solution resulting from the application of the JKTEBOP ...only the I-band light curve, and values of the mass ... See full document
8
Massive Stellar X ray Sources in the Galactic Center
... to the X-ray population has revealed a growing number of massive stellar X-ray sources near the Galactic center (GC), outside of the well known Arches, Quintuplet and Sgr A ∗ star ... See full document
5
Perspectives in processing large amounts of information using Cloud
... process large amounts of ...generally large, and the calculations have to be distributed through many machines in order to be able to do it in a short period of ...time. The fact ... See full document
4
Near infrared photometry of Galactic planetary nebulae with the VVV Survey
... thank the anonymous referee whose very useful re- marks helped us to substantially improve this ...improve the paper. This research has made use of the Aladin and SIMBAD database, operated at CDS, ... See full document
10
Neutron energy distribution and temporal correlations with hard x ray emission from a hundreds of joules plasma focus device
... to the differences in photon and neutron velocities, the first pulse represents the hard x-rays’ detection, whereas the second cor- responds to the ...from ... See full document
7
La imagen radiolgica de la tuberculosis pulmonar en pacientes con farmaco resistencia Estudio comparativo
... 18. Spencer D, Yagan R, Blinkhorn R, Spagnuolo PJ. Anterior segment upper lobe tuberculosis in adult. Occurrence in primary and reactivation disease. Chest 1990; 97: 384-388. 19. Christensen EE, Dietz GW, ... See full document
5
16641917
... detected in the distal-most blastema, a region of reduced proliferation rate compared with more proximal areas of the blastema (Akimenko et ...differences in expression for both msxC and msxE/1 ... See full document
12
THE ARAUCARIA PROJECT DETERMINATION OF THE LARGE MAGELLANIC CLOUD DISTANCE FROM LATE TYPE ECLIPSING BINARY SYSTEMS I OGLE 051019 64 685812 3
... with the Warsaw 1.3 m telescope at Las Campanas Observatory in the course of the second and third phases of the OGLE project (Wyrzykowski et ...secured. In order to obtain ... See full document
5
A new optical polarization catalog for the small magellanic cloud: the magnetic field structure
... of the SMC – LMC – MW system seems to have generated two interesting structures — the Magellanic Stream and the Magellanic ...illustrated in the HI column density map ( ... See full document
19
The Contact Structure in the Space of Light Rays
... that in dimension 3 this dual approach to causality becomes very ...if the dimension of spacetime is m = 3, the dimension of the space of light rays is also 2m − 3 = 3 and the ... See full document
27
TítuloRiding the cloud Information and architectural representation in the post digital age
... of the fields in which the impact of digital technologies has had most importance is that of the architectural survey of cultural heritage, with a continuous evolution of ... See full document
8
Heavily Obscured AGN in Star Forming Galaxies at z sime 2
... study the possible effects of the spread in redshift of our sample we also performed X-ray stacking in the approximate rest-frame, ...correct the incident photon energy ... See full document
18
A cost-effective methodology applied to videoconference services over hybrid clouds
... provider, which has special deals in storage services (named X stor ). Then, given the architecture explained before and basing on the Cloud Price Calculator we mentioned in Section 1[r] ... See full document
7
Galactic Planetary Nebulae with Wolf-Rayet Nuclei III. Kinematical Analysis of a Large Sample of Nebulae
... planetary nebulae (hereinafter WRPNe) and their central stars with interesting new ...that the physical properties and chemical abundances of WRPNe were not dif- ferent from those of non-WRPNe, except for ... See full document
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