Milky Way Galaxy
AGB Stars Migration fom the Central of the Milky Way Galaxy to Our Sun’s Birthplace and Its Relation with Silicon Carbide Grains
... the Galaxy bulge and examines possibility of migration to outer regions by scattering off molecular ...the Galaxy and will shed new light unto the age and the chemical evolution of the Milky ...
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Schönrich, Ralph (2011): Structure, Kinematics and Chemistry of the Milky Way Galaxy. Dissertation, LMU München: Fakultät für Physik
... Investigations into the structure of the model yielded a surprise for Galactic kinematics. At least since the work of Delhaye (1965) it was common knowledge that the Local Standard of Rest (LSR) could be determined via ...
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The Basic Principles of Creation of Habitable Planets around Stars in the Milky Way Galaxy
... The principle of habitable planets creation of near stars in our galaxy was developed. It was shown that the Earth and the Moon formed as a result of thermal nuclear ex- plosion (TNE) after a collision with a ...
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Modelling the Milky Way as a dry Galaxy
... most 50 % of the snapshots, we observed a velocity structure similar to the Hercules stream. The radius at which we most frequently see the Hercules-like stream is slightly further out than the outer Lindblad resonance. ...
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Sixth Edition
... Jones, May, and Smith (2009) stated the composition of the moon originates from another galaxy other than the Milky Way Galaxy.. The moon, according to Jones et al., was most likely mov[r] ...
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Streaming motions and kinematic distances to molecular clouds
... Simulations allow us to compare actual distances with kinematic estimates. Several works using global simulations of a Milky Way galaxy concluded that it is feasible to reconstruct the structure to ...
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H_2 and its relation to CO in the LMC and other magellanic irregular galaxies
... on observed quantities independent of the actual spatial or kinematical distribution of the molecular material. It has this property in common with the methods used by Bloemen et al. (1986) and Bloemen et al. (1990) to ...
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The Formation and Dynamical Evolution of Young Star Clusters
... the Milky Way Galaxy tend to form embedded clusters that evolve to resemble open ...the Milky Way but are typical in starburst galaxies, form massive, young star ...
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Sixth Edition
... Jones, May, and Smith (2009) stated the composition of the moon originates from another galaxy than the Milky Way Galaxy.. The moon, according to Jones et al., was most likely moved to[r] ...
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Relativity of Speed of Light with Speed of Universe Expansion
... of MILKY WAY galaxy on account of universe expansion is approximately 299,792 km/s ...of MILKY WAY galaxy is on account of velocity of MILKY WAY galaxy on ...
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Lesson 15 - Space Review Jeopardy.ppt
... These very distant objects look like faint stars, but give off 100 times more energy than the Milky. Way galaxy.[r] ...
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The Milky Way and its gas: Cold fountains and accretion
... The disk-halo transition zone in spiral galaxies is a lively place. Energetic events associated with star formation can lift gas several kpc into the halo [9, 14]. Some spirals have an associated population of ...
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The law of interstellar extinction in the southern Milky Way
... the Galaxy, Johnson suggested that the distance to the Galactic Centre would be reduced from 10 to about 8 kpc, and that O o r t ’s constant A would be increased from 15 to about 20 kra/sec/kpc, A discrep ancy ...
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Physical Properties of Molecular Clouds at 2 pc Resolution in the Low-metallicity Dwarf Galaxy NGC 6822 and the Milky Way
... Table 2 summarizes the properties of our target regions. All four inner regions have been studied extensively, and two of them, Hubble V and X ( our ALMA Fields 2 and 1 ) , are classic targets for extragalactic studies ...
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OGLE Cepheids and RR Lyrae stars in the Milky Way
... In 2013 a new OGLE long-term survey – OGLE Galaxy Variability Survey (OGLE GVS) – was initiated in the frame of the OGLE-IV phase. An area of about 2000 square degrees in the sky is regularly monitored. The survey ...
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Faint (and bright) variable stars in the satellites of the Milky Way
... The importance of finding and characterizing dwarf Cepheid stars resides in their potential use as standard candles. They are known to follow a clear period-luminosity (PL) relationship ([13]). It has been suggested that ...
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Towards the big picture of the Milky Way bulge
... In [5] we used the sample analyzed in [1] as part of a project aimed to provide a spectroscopic characterization of the Galactic bulge. The sample consists of 650 K giant stars spectra, from 3 fields along the Bulge ...
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Results of the ESO-SEST key programme: CO in the Magellanic Clouds. VI. The 30 DOR Complex
... in Milky Way molecular clouds (except for the line ...in Milky Way molecular clouds suggests that many of these physical conditions are com- parable in the LMC and the Milky ...
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IRAS galaxies behind the Milky Way
... IRAS Galaxies Behind The Milky Way by Frank de Ruyter A thesis submitted for the degree of Master of Science of The Australian National University 16 December 1997 Mount Stromlo and Siding Spring Obse[.] ...
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Constraining the formation of the Milky Way: Ages
... With 4MOST we aim at maximizing the scientific return of Gaia, thanks to additional chemical abundance information for stars fainter than ∼14 mag, and radial velocities with a precision better then 2 km/s for stars in ...
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