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MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 02/2020, Volume 492, Issue 2, pp. 2481 - 2496
IRS 13E is an enigmatic compact group of massive stars located in projection only 3.6 arcsec away from Sgr A*. This group has been suggested to be bounded by... 
PASCHEN-ALPHA SURVEY | MASSIVE STARS | X-rays: general | hydrodynamics | stars: winds, outflows | SUPERMASSIVE BLACK-HOLE | SGR-A-ASTERISK | stars: Wolf-Rayet | PROPER MOTIONS | Galaxy: centre | ASTRONOMY & ASTROPHYSICS | IONIZED-GAS | CENTRAL PARSEC | VELOCITY-FIELD | CHEMICAL ABUNDANCES | ACCRETION FLOW
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 02/2017, Volume 465, Issue 2, pp. 1409 - 1442
Hot, tenuous advection-dominated accretion flows around black holes are ideal sites for the Fermi acceleration of relativistic particles at standing shock... 
RELATIVISTIC OUTFLOWS | ADVECTION-DOMINATED ACCRETION | acceleration of particles | RADIO GALAXY M87 | accretion, accretion discs | RADIATION | SGR-A-ASTERISK | RAY-MODIFIED SHOCKS | FUNCTION ENERGY-DISTRIBUTION | STANDING SHOCKS | galaxies: active | ASTRONOMY & ASTROPHYSICS | JET | astroparticle physics | CYGNUS X-1 | shock waves
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 12/2019, Volume 490, Issue 4, pp. 4606 - 4621
The Event Horizon Telescope (EHT), now with its first ever image of the photon ring around the supermassive black hole of M87, provides a unique opportunity to... 
ADVECTION-DOMINATED ACCRETION | SGR A-ASTERISK | SCALE STRUCTURE | RAY-EMISSION | accretion, accretion discs | BLACK-HOLE MASS | ASTRONOMY & ASTROPHYSICS | CENTRAL PARSECS | XMM-NEWTON OBSERVATIONS | RADIATIVE EFFICIENCY | RADIO-EMISSION | galaxies: nuclei | CYGNUS X-1 | Physics - High Energy Astrophysical Phenomena
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 12/2019, Volume 490, Issue 4, pp. 5820 - 5831
Studies of the Galactic Centre suggest that in situ star formation may have given rise to the observed stellar population near the central supermassive black... 
NUCLEAR CLUSTERS | Galaxy: evolution | FORMATION HISTORY | SEGREGATION | Galaxy: formation | SGR-A-ASTERISK | stars: formation | ORIGIN | EVOLUTION | Galaxy: centre | ASTRONOMY & ASTROPHYSICS | CENTRAL PARSEC | BINARIES | Galaxy: nucleus | stars: kinematics and dynamics | MASSIVE BLACK-HOLE | SIMULATIONS
Journal Article
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 12/2019, Volume 887, Issue 2, p. 167
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 10/2019, Volume 489, Issue 1, pp. 52 - 77
Numerical models of gas inflow towards a supermassive black hole (SMBH) show that star formation may occur in such an environment through the growth of a... 
MOLECULAR CLOUDS | radiative transfer | hydrodynamics | ACCRETION DISKS | SGR-A-ASTERISK | RADIATIVE-TRANSFER | stars: formation | EVOLUTION | Galaxy: centre | ASTRONOMY & ASTROPHYSICS | CENTRAL PARSEC | YOUNG STARS | GALACTIC-CENTER | SIMULATIONS | FEEDBACK
Journal Article
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 09/2019, Volume 882, Issue 2, p. 82
Journal Article
PHYSICAL REVIEW D, ISSN 2470-0010, 08/2019, Volume 100, Issue 4, p. 1
Journal Article
by Porth, O and Chatterjee, K and Narayan, R and Gammie, CF and Mizuno, Y and Anninos, P and Baker, JG and Bugli, M and Chan, CK and Davelaar, J and Del Zanna, L and Etienne, ZB and Fragile, PC and Kelly, BJ and Liska, M and Markoff, S and McKinney, JC and Mishra, B and Noble, SC and Olivares, H and Prather, B and Rezzolla, L and Ryan, BR and Stone, JM and Tomei, N and White, CJ and Younsi, Z and Akiyama, K and Alberdi, A and Alef, W and Asada, K and Azulay, R and Baczko, AK and Ball, D and Balokovic, M and Barrett, J and Bintley, D and Blackburn, L and Boland, W and Bouman, KL and Bower, GC and Bremer, M and Brinkerink, CD and Brissenden, R and Britzen, S and Broderick, AE and Broguiere, D and Bronzwaer, T and Byun, DY and Carlstrom, JE and Chael, A and Chatterjee, S and Chen, MT and Chen, YJ and Cho, I and Christian, P and Conway, JE and Cordes, JM and Crew, GB and Cui, YZ and De Laurentis, M and Deane, R and Dempsey, J and Desvignes, G and Doeleman, SS and Eatough, RP and Falcke, H and Fish, VL and Fomalont, E and Fraga-Encinas, R and Freeman, B and Friberg, P and Fromm, CM and Gomez, JL and Galison, P and Garcia, R and Gentaz, O and Georgiev, B and Goddi, C and Gold, R and Gu, MF and Gurwell, M and Hada, K and Hecht, MH and Hesper, R and Ho, LC and Ho, P and Honma, M and Huang, CWL and Huang, L and Hughes, DH and Ikeda, S and Inoue, M and Issaoun, S and James, DJ and Jannuzi, BT and Janssen, M and Jeter, B and Jiang, W and Johnson, MD and ... and Event Horizon Telescope Collaborat and The Event Horizon Telescope Collaboration and Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, ISSN 0067-0049, 08/2019, Volume 243, Issue 2, p. 26
Journal Article
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 08/2019, Volume 880, Issue 2, p. 87
In various fields of physics and astronomy, access to experimental facilities or to telescopes is becoming more and more competitive and limited. It therefore... 
MILKY | methods: statistical | DISTANCE | methods: data analysis | PROPER MOTIONS | SGR A-ASTERISK | ASTRONOMY & ASTROPHYSICS | STARS | Galaxy: center | SUPERMASSIVE BLACK-HOLE
Journal Article
Journal Article