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Данные предоставлены сервисом semrush
Данные linkpad ( 10 Февраля 2015 ) | |
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Внешние ссылки главной страницы ( 63 ) | |
groups.google.com/forum/#!forum/kromeusers | Get Help |
gnu.org/licenses/gpl-3.0.txt | GNU-licensed |
bitbucket.org/tgrassi/krome/overview | Bitbucket |
arxiv.org/abs/1311.1070 | KROME Paper |
bitbucket.org/tgrassi/krome/wiki/Home | User Guide |
bitbucket.org/tgrassi/krome/wiki/Get_started | Quick Start |
ui.adsabs.harvard.edu/#abs/arXiv:1905.12639 | Planet-forming material in a protoplanetary disc: the interplay between chemical evolution and pebble drift |
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2019MNRAS.... | Ly α emission from galaxies in the Epoch of Reionization |
adsabs.harvard.edu/cgi-bin/nph-data_query?doi=10.1093/mnras/... | Deep into the structure of the first galaxies: SERRA views |
ui.adsabs.harvard.edu/abs/2019MNRAS.485.3352L/abstract | Black hole formation in the context of dissipative dark matter |
ui.adsabs.harvard.edu/abs/2019arXiv190303637S/abstract | The role of gas fragmentation during the formation of supermassive black holes |
ui.adsabs.harvard.edu/abs/2019arXiv190300017G/abstract | Intermittent fragmentation and statistical variations during gas collapse in magnetised atomic cooling haloes |
adsabs.harvard.edu/abs/2019arXiv190102464L | High-redshift quasars and their host galaxies I: kinematical and dynamical properties and their tracers |
adsabs.harvard.edu/abs/2019MNRAS.484.1687L | chemistry in galaxy simulations: an improved supernova feedback model |
adsabs.harvard.edu/doi/10.1093/mnras/sty2560 | Developing a self-consistent AGB wind model: I. Chemical, thermal, and dynamical coupling |
adsabs.harvard.edu/abs/2018arXiv180905541F | Lampray: Multi-group long characteristics ray tracing for adaptive mesh radiation hydrodynamics |
adsabs.harvard.edu/abs/2018MNRAS.479..667R | The formation of protostellar binaries in primordial minihaloes |
arxiv.org/abs/1808.10184 | H2 chemistry in galaxy simulations: an improved supernova feedback model |
arxiv.org/abs/1710.01315 | The natural emergence of the correlation between H2 and star formation rate surface densities in galaxy simulations |
arxiv.org/abs/1710.01302 | The effect of non-equilibrium metal cooling on the interstellar medium |
adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1709.04013 | Fast deuterium fractionation in magnetized and turbulent filaments |
adsabs.harvard.edu/abs/2017arXiv170802046B | ortho-to-para conversion on grains: A route to fast deuterium fractionation in dense cloud cores? |
adsabs.harvard.edu/abs/2017arXiv170704259P | The impact of chemistry on the structure of high-z galaxies |
arxiv.org/abs/1707.03419 | Massive Black Holes from Dissipative Dark Matter |
arxiv.org/abs/1703.01201v1 | evolution in turbulent and magnetized cloud cores |
adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1702.03227 | Modelling the chemistry of star forming filaments - II. Testing filament characteristics with synthetic observations |
adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1607.05461 | H (n=4,6,8) in dense molecular clouds |
adsabs.harvard.edu/abs/2016arXiv160601229G | A detailed framework to incorporate dust in hydrodynamical simulations |
adsabs.harvard.edu/abs/2016arXiv160104525B | The formation of the primitive star SDSS J102915+172927: effect of the dust mass and the grain-size distribution |
adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1510.07016 | A chemical model for the interstellar medium in galaxies |
adsabs.harvard.edu/abs/2015arXiv151008346M | Connecting the evolution of thermally pulsing asymptotic giant branch stars to the chemistry in their circumstellar envelopes |
adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1510.06544 | Modelling the chemistry of star forming filaments |
adsabs.harvard.edu/abs/2015arXiv151002788L | Witnessing the birth of a supermassive protostar |
adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1509.07034 | Impact of dust cooling on direct collapse black hole formation |
adsabs.harvard.edu/abs/2015MNRAS.451.2352K | Seeding High Redshift QSOs by Collisional Runaway in Primordial Star Clusters |
adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1504.00263 | Assessing inflow rates in atomic cooling halos: implications for direct collapse black holes |
adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1410.4061 | The origin of spin in galaxies: clues from simulations of atomic cooling haloes |
adsabs.harvard.edu/abs/2015A%26A...578A.118L | The formation of supermassive black holes in rapidly rotating disks |
adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1408.3061 | How realistic UV spectra and X-rays suppress the abundance of direct collapse black holes |
adsabs.harvard.edu/abs/2015MNRAS.449...77L | Disc fragmentation and the formation of Population III stars |
adsabs.harvard.edu/abs/2015arXiv150406296S | The chemical evolution of self-gravitating primordial disks |
adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1311.1070 | KROME - a package to embed chemistry in astrophysical simulations |
adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1408.1253 | Effects of turbulence and rotation on protostar formation as a precursor to seed black holes |
adsabs.harvard.edu/abs/2014MNRAS.441.2181B | Dark-matter halo mergers as a fertile environment for low-mass Population III star formation |
adsabs.harvard.edu/abs/2014arXiv1406.4450B | Formation of carbon-enhanced metal-poor stars in the presence of far ultraviolet radiation |
adsabs.harvard.edu/abs/2014arXiv1406.1465L | The formation of massive primordial stars in the presence of moderate UV backgrounds |
adsabs.harvard.edu/abs/2014arXiv1404.5773L | A UV flux constraint on the formation of direct collapse black holes |
adsabs.harvard.edu/abs/2014A%26A...561A..13B | three-body rates and initial conditions |
adsabs.harvard.edu/abs/2013MNRAS.436.2722S | : a quantum modelling of the process |
adsabs.harvard.edu/abs/2013MNRAS.434L..36B | Impact of an accurate modelling of primordial chemistry in high-resolution studies |
adsabs.harvard.edu/abs/2013arXiv1306.4857B | CH+ depletion by atomic hydrogen: accuracy of new rates in photo-dominated and self-shielded environments |
adsabs.harvard.edu/abs/2013EGUGA..15.3388G | Exploring planetary biomarkers: a new physical method coupled with new computational tool |
phys.org/news/2014-07-astrophysicists-formation-oldest-known... | phys.org |
snm.ku.dk/english/news/all_news/2014/2014.11/scientists-mode... | SNM |
uni-goettingen.de/en/3240.html?cid=4863 | UniGoe |
media.inaf.it/2014/07/23/simulazione-stella-keller/ | INAF (Italian) |
iopscience.iop.org/article/10.1088/2041-8205/790/2/L35/meta | ApJL |
arxiv.org/abs/1406.4450 | arXiv |
starplan.dk/ | <img> |
nbi.ku.dk/ | <img> |
ism-spp.de/ | <img> |
hs.uni-hamburg.de/index.php?lang=en | <img> |
mrova.com | mRova |
Внутренние ссылки главной страницы ( 8 ) | |
index.php | KROME PACKAGE |
#aboutus | many others |
bootcamp/index.php | here |
bootcamp/2015/ | here |
bootcamp/2016/ | here |
bootcamp/2014/index.php | here |
bootcamp/2014/ | 2014 edition |
test/ | Download |
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