Difference between revisions of "Main Page"
From Astrophysics Journal Club
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== 2018-04-17 == | == 2018-04-17 == | ||
| − | * J An: | + | * J An: [https://www.nature.com/articles/nature25767 A galaxy lacking dark matter] |
| − | + | * Jinho Kim: [https://arxiv.org/abs/1710.05891 Can we distinguish low mass black holes in neutron star binaries?] | |
== 2018-04-10 == | == 2018-04-10 == | ||
| − | * S Ahn: | + | * S Ahn: [https://www.nature.com/articles/nature25029.pdf A density cusp of quiescent X-ray binaries in the central parsec of the Galaxy] |
| − | + | ** cf. [https://arxiv.org/pdf/0810.4674v1.pdf Stars orbiting around Sgr A*] | |
| − | + | ** cf. [http://2.bp.blogspot.com/-BEYTIq-0RFQ/Vc4R7K5O2nI/AAAAAAAABBU/wNvzcIH3Ffs/s1600/scr00144.jpg Figure] | |
| − | + | ||
* Thiem Hoang: [https://arxiv.org/abs/1804.02250v1 Absorption by Spinning Dust: a Contaminant for High-Redshift 21 cm Observations, arXiv:11804.02250, by Draine and Miralda-Escude] | * Thiem Hoang: [https://arxiv.org/abs/1804.02250v1 Absorption by Spinning Dust: a Contaminant for High-Redshift 21 cm Observations, arXiv:11804.02250, by Draine and Miralda-Escude] | ||
Revision as of 02:22, 17 April 2018
2018-04-17
- J An: A galaxy lacking dark matter
- Jinho Kim: Can we distinguish low mass black holes in neutron star binaries?
2018-04-10
- S Ahn: A density cusp of quiescent X-ray binaries in the central parsec of the Galaxy
- cf. Stars orbiting around Sgr A*
- cf. Figure
2018-04-03
- J An:
2018-03-27
- Jinho Kim: Relativistic Low Angular Momentum Accretion: Long Time Evolution of Hydrodynamical Inviscid Flows
2018-03-13
- Yeong-Bok Bae: Fundamentals of the orbit and response for TianQin