Feb 28 2016 Monoceros - The Unicorn By NGC /IC Number Catalog IC IC IC IC IC IC IC IC IC 446 447 448 466 487 2167 2169 2172 2177 M Her Object Type Nebula bipolar Non-Existent Nebula R Nebula E+R Non-Existent Non-Existent Nebula R Non-Existent Nebula E Non-Existent Nebula R Mag Alias/Notes 12 IC 2167 IC 2169 NGC 2494 UGC 4141 MCG 0-21-1 CGCG 3-2 IRAS 7565-30 PGC 22377 IC 2169 NGC 2282 ... Open Cl 8.0 II 2 p n Pl Neb 3b+4 Non-Existent Open Cl 9.0 III 3 p Open Cl cluster? ...

MATSYM - symbolic matrix processor . ... To use the program you will need a MAT file (liked CIR file: "User manual for CIRSYM program") of your system. ... In first string of MAT file enter any text you want to be the title of your system. ... Starting from string 2 (if is not comments - "*") enter the system element name, incident row and column and, optionally, its value. ... To generate a solution, run MATSYM.exe and enter "system_file_name.CIR" or click on the "ENTER" (in "MAT" case). ...

... 3 ­ Sternberg State Astronomical Institute, Moscow, :jeanna@sai.msu.ru The graphic method of the analysis of an arrangement of linear structural elements on geographical and geological maps of continents (A.V.Dolitsky, [1]) has allowed to find out global stress fields of the past and among them one which directions (the main normal and maximal tangents) describe more than 80 % of all linear elements of a relief. ... The found poles share program way on density of an arrangement on 3-4 groups. ...

http ://vo.astronet.ru/arxiv/index.php?offset=0 number=100 sort=date query=sn astro-ph articles matcing the query en-us Sun, 10 Apr 2016 03:29:43 MSK Sun, 10 Apr 2016 03:29:43 MSK karpov@sao.ru karpov@sao.ru http :// arxiv.org / abs /1604.01930 oai : arXiv.org :1604.01930 http :// arxiv.org / abs /1604.02095 oai : arXiv.org :1604.02095 http :// arxiv.org / abs /1603.07163 oai : ...

... We address a question if globular clusters (GC) in a protogalaxy could for some time evolve chemically as isolated systems, enriching themselves with heavy elements produced in first supernova events that follow initial star formation. We determine both the critical mass of a protoglobular cluster that is needed to retain the ejecta of the very first supernova, and the critical energy (i.e., number of supernovae) that is needed to expel the residual gas from a cluster of a given mass. ...

... GCR and SCR are primary cosmic rays. 10-15 years after the discovery of cosmic radiation (1919) there emerged two main avenues of investigation in the physics of cosmic rays (CR): 1) nuclear - elucidation of the origin of elementary particles and nuclear interactions; and 2) astrophysical (space physics) - solution of the problem related to the origin and variations (changes in intensity) of CR. ... Besides, the CR flux in interplanetary space is, strictly speaking, not isotropic. ...