[PDF] Top 20 Polarisation in the galaxy and the large Magellanic Cloud
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Polarisation in the galaxy and the large Magellanic Cloud
... Considering that the pola ris a tion due to our Galaxy, in the field of Larg e Magellanic Cloud is less than 0.002 mag and that for the Cloud stars the mean error in the determination of[r] ... See full document
236
A survey for stellar relics of galaxy formation in the large Magellanic cloud
... The AMR of various populations within the LMC have been studied by several authors (e.g. Cole et al. (2005); Carrera et al. (2011); Piatti et al. (2012)). Based on the AMR derived from red giant stars in the central bar, ... See full document
168
Infrared composition of the Large Magellanic Cloud
... Dust is a common ingredient of the interstellar medium (ISM) of galaxies. In the imaging obtained by optical ob- servatories, such as the Hubble Space Telescope, dust man- ifests itself as dark lanes or patches that are ... See full document
5
A multi-frequency analysis of radio supernova remnants and their environments in Sculptor Group SD Galaxy NGC 300 and the Small Magellanic Cloud
... of Large Magellanic Cloud radio supernova remnants”, published in the Monthly Notices of the Royal Astronomical Society (MNRAS), 2008, volume 383, pages ... See full document
18
Star cluster formation history along the minor axis of the Large Magellanic Cloud
... regions of the LMC were disturbed by ram pressure effects due to the motion of the LMC in the MW halo. Particularly, Salem et al. (2015) found evidence that the LMC’s gaseous disc has recently experienced ram pressure ... See full document
11
The nature and kinematics of long-period variables in the Large Magellanic Cloud
... After stars of 0.5 to 9 M® have exhausted the He in their cores, He burning continues in a shell about the C -0 core, which in turn is surrounded by a H burning shell. Initially, the He-burning shell contracts and ... See full document
283
Thermal and Non-Thermal Contributions to the X-ray Spectrum of Large Magellanic Cloud Supernova Remnants
... The X-ray spectral analysis package XSPEC contains many models useful for anaylsis, and allows for external models to be linked to it. Before reviewing models of thermal emission found in XSPEC, we need to discuss some ... See full document
189
Milky way halo objects, IC 4499 and the large magellanic cloud
... a large sample of LMC disk field and bar field stars to establish the nature of those two primary morphologies, disk and ...disk galaxy have been ... See full document
269
On the dynamics of the Small Magellanic Cloud through high resolution ASKAP HI observations
... the large asymmetries in the observed velocity field, our completely symmetric tilted-ring model does a fairly good job in reproducing the overall rotation behaviour of the ...the large discrepancies from ... See full document
15
A multi-frequency analysis of radio supernova remnants and their environments in Sculptor Group SD Galaxy NGC 300 and the Small Magellanic Cloud
... Chapter 2 was originally published as a “Multi-frequency Study of extragalactic supernova remnants and H regions. Sculptor group Sd galaxy NGC 300”, in Astronomy and Astrophysics, 2004, volume 425, pages ... See full document
235
Sasaki, Manami (2002): X-rays tracing the star formation history of the Magellanic clouds. Dissertation, LMU München: Fakultät für Physik
... our Galaxy with the largest occurrence in the proximity of the Galactic center as well as in the spiral ...the Galaxy ranges from 100 to 200 ...spiral galaxy M 31, the Andromeda galaxy, giant ... See full document
175
Photometric metallicity map of the Small Magellanic Cloud
... the Magellanic Cloud Photometric Survey (MCPS) and OGLE III photometric ...a large area of the galaxy, unlike the spectroscopic method, which can over only rela- tively small ...show ... See full document
19
Properties of Anomalous and Type II Cepheids in the Small and Large Magellanic Clouds
... Small Magellanic Cloud (SMC) and Large Magellanic Cloud (LMC) give us the possibility to study individual variable star types in a new ... See full document
5
Ten eclipsing binaries in the Small Magellanic Cloud: fundamental parameters and Cloud distance
... This is a rather venerable scale which, at these tem- peratures, is derived in large part from studies by Conti (1973) and by Underhill et al. (1979), which in turn are not above criticism (being based on ... See full document
18
Multiwavelength observations of nova SMCN 2016 10a one of the brightest novae ever observed
... We found several sources less than ∼ 1.0 00 from the nova in archival data from: USNO-B1 catalogue (Monet et al. 2003) (B = 20.17 and R = 20.0); the Magel- lanic Cloud Photometric Survey (MCPS; Zaritsky et al. ... See full document
31
Grimm, Hans-Jakob (2003): X-ray binaries in the Milky Way and other galaxies. Dissertation, LMU München: Fakultät für Physik
... Progress in the number of distance determinations and identifications of secondary stars in X-ray binaries in the last decade opens the opportunity to study the 3-D distribution of XRBs in more detail than was previously ... See full document
128
The employee's productivity in the health care sector in Poland and their impact on the treatment process of patients undergoing elective laparoscopic cholecystectomy
... Through engagement of medical employees availability of 24 hours doctors in the ward, explaining to patients about the drug therapy by medical professional, and informing patients abo[r] ... See full document
11
The Jews and the Muslims: A Study in the Similarity between “The Merchant of Venice” and an Islamic Story entitled “The Merchant and the Jew”
... As for the cultural aspects of the city, Venice, we can mention the fact that this city was highly under the influence of the Islamic world. The closeness between the Islamic world and the Venetians is seen through a ... See full document
6
Improving the Innovative Strategy of Interaction of Large Industrial Enterprises and Small Entrepreneurship in the Agro-industrial Sector
... contractors. Consequently, interests of such diverse entities will also be different, and their contribution to an inter-firm strategic interaction organization will also be different. Therefore, we can conclude that ... See full document
9
A Survey on the Mechanisms used for the Detection and the Prevention of the Selective Forwarding and Black Hole Attacks in the WSNs
... a large amount of disseminated sensor nodes in meticulous surroundings for monitoring and ...a large amount cases, these minute sensors nodes are operational with a processor, transmitter, radio ... See full document
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