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| * ''Possible Origin of the G2 Cloud from the Tidal Disruption of a Known Giant Star by Sgr A*'' [[http://arxiv.org/abs/1312.4386| Guillochon et al. 2014, arXiv/1401.2990]] | * ''Possible Origin of the G2 Cloud from the Tidal Disruption of a Known Giant Star by Sgr A*'' [[http://arxiv.org/abs/1401.2990| Guillochon et al. 2014, arXiv/1401.2990]] * ''Spitzer/IRAC Observations of the Variability of Sgr A* and the Object G2 at 4.5 microns'' [[http://arxiv.org/abs/1408.1951| Hora et al. 2014, arXiv/1408.1951]] * ''Magnetized Gas Clouds can Survive Acceleration by a Hot Wind'' [[http://arxiv.org/abs/1409.6719| McCourt et al. 2014, arXiv/1409.6719]] |
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| * ''The Galactic Center cloud G2 and its gas streamer'' [[http://arxiv.org/abs/1407.4354| Pfuhl et al. 2014]] | |
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| * ''No Microwave Flare of Sagittarius A* around the G2 Periastron Passing'' [[http://arxiv.org/abs/1411.0746| Tsuboi et al., arXiv/1411.0746]] * ''Monitoring the Dusty S-Cluster Object (DSO/G2) on its Orbit towards the Galactic Center Black Hole'' [[http://arxiv.org/abs/1410.8731| Valencia-S. et al., arXiv/1410.8731]] * ''Detection of Galactic Center source G2 at 3.8 μm during periapse passage'' [[http://arxiv.org/abs/1410.1884| Witzel et al., arXiv/1410.1884]] |
List of publications on G2
Papers for which the main topic is G2
Simulating the effect of the Sgr A* accretion flow on the appearance of G2 after pericenter Abarca, Sadowski & Sironi, arXiv/1309.2313
3D Moving-Mesh Simulations of Galactic Center Cloud G2 Anninos et al. 2012, ApJ, 759, 132
Hydrodynamic simulations of a compact source scenario for the Galactic Center cloud G2 Ballone et al., arXiv/1305.7238
G2 can Illuminate the Black Hole Population near the Galactic Center Bartos et al., arXiv/1302.3220
Physics of the Galactic Center Cloud G2, on Its Way toward the Supermassive Black Hole Burkert et al. 2012, ApJ, 750, 58
Radio Synchrotron Emission from the Bow Shock of G2 Crumley & Kumar, arXiv/1309.1762
Multiple accretion events as a trigger for Sgr A* activity Czerny et al., arXiv/1306.0900
Colliding with G2 near the Galactic Centre: a geometrical approach de la Fuente Marcos & de la Fuente Marcos, arXiv/1306.4921
The infrared K-band identification of the DSO/G2 source from VLT and Keck data Eckart et al., arXiv/1311.2753
A gas cloud on its way towards the supermassive black hole at the Galactic Centre Gillessen et al. 2012, Nature, 481, 51
New observations of the gas cloud G2 in the Galactic Center Gillessen et al. 2013, ApJ, 763, 78
Pericenter passage of the gas cloud G2 in the Galactic Center Gillessen et al. 2013, ApJ, 774, 44
Observations of the gas cloud G2 in the Galactic Center Gillessen et al. 2013, arXiv/1312.4386
Possible Origin of the G2 Cloud from the Tidal Disruption of a Known Giant Star by Sgr A* Guillochon et al. 2014, arXiv/1401.2990
Spitzer/IRAC Observations of the Variability of Sgr A* and the Object G2 at 4.5 microns Hora et al. 2014, arXiv/1408.1951
Magnetized Gas Clouds can Survive Acceleration by a Hot Wind McCourt et al. 2014, arXiv/1409.6719
A nova origin of the gas cloud at the Galactic Center ? Meyer & Meyer-Hofmeister 2012, A&A, 546, L2
A Star Disrupted by a Stellar Black Hole as the Origin of the Cloud Falling toward the Galactic Center Miralda-Escudé 2012, ApJ, 756, 86
Astrophysics: The final plunge Morris 2012, Nature, 481, 32
The Galactic Center Weather Forecast Mościbrodzka et al. 2012, ApJ, 752, L1
Disruption of a Proto-Planetary Disk by the Black Hole at the Milky Way Centre Murray-Clay & Loeb 2012, Nat. Commun. 3:1049 doi: 10.1038/ncomms2044
Radio Synchrotron Emission from a Bow Shock around the Gas Cloud G2 Heading toward the Galactic Center Narayan, Özel & Sironi 2012, ApJ, 757, L20
The Galactic Center cloud G2 and its gas streamer Pfuhl et al. 2014
Keck Observations of the Galactic Center Source G2: Gas Cloud or Star? Phifer et al., arXiv/1304.5280
Radio light curves during the passage of cloud G2 near Sgr A* Sadowski et al., arXiv/1301.3906
Location of the bow shock ahead of cloud G2 at the Galactic Center Sadowski et al., arXiv/1303.3893
Flaring up of the Compact Cloud G2 during the Close Encounter with Sgr A* in Summer 2013 Saitoh et al., arXiv/1212.0349
Simulations of the Origin and Fate of the Galactic Center Cloud G2 Schartmann et al. 2012, ApJ, 755, 155
The Galactic Center Cloud G2 -- a Young Low-Mass Star with a Stellar Wind Scoville & Burkert, arXiv/1302.6591
The Cloudy Life of the Galactic Center Shcherbakov, arXiv/1309.2282
No Microwave Flare of Sagittarius A* around the G2 Periastron Passing Tsuboi et al., arXiv/1411.0746
Monitoring the Dusty S-Cluster Object (DSO/G2) on its Orbit towards the Galactic Center Black Hole Valencia-S. et al., arXiv/1410.8731
Detection of Galactic Center source G2 at 3.8 μm during periapse passage Witzel et al., arXiv/1410.1884
Signatures of an Encounter Between the G2 Cloud and a Jet from Sgr A* Yusef-Zadeh et al., arXiv/1303.3969
Dust-enshrouded star near supermassive black hole: predictions for high-eccentricity passages near low-luminosity galactic nuclei Zajacek et al., arXiv/1403.5792
Papers commenting on G2
Near-infrared proper motions and spectroscopy of infrared excess sources at the Galactic Center Eckart et al. 2013, A&A, 551A, 18
The Galactic Center as a Paradigm for Low Luminosity Nuclei? The K-band identification of the DSO/G2 source from VLT and Keck data Eckart et al., arXiv/1311.2743
Galactic center research: manifestations of the central black hole Morris, Meyer & Ghez 2012, RAA, 12, 995
Coupled jet-disk model for Sgr A*: explaining the flat-spectrum radio core with GRMHD simulations of jets Moscibrodzka & Falcke, arXiv/1310.4951
Secular Evolution Of Binaries Near Massive Black Holes: Formation of compact binaries, merger/collision products and G2-like objects Prodan, Antonini & Perets, arXiv/1405.6029
Papers mentioning G2
The X-ray flaring properties of Sgr A* during six years of monitoring with Swift Degenaar et al., arXiv/1210.7237
In Situ Formation of SgrA* Stars Via Disk Fragmentation: Parent Cloud Properties and Thermodynamics Mapelli et al. 2012, ApJ, 749, 168
A formal method for identifying distinct states of variability in time-varying sources: SgrA* as an example Meyer et al., arXiv/1403.5289
Traces of past activity in the Galactic Centre Ponti et al., arXiv/1210.3034
Compact Dusty Clouds in a Cosmic Environment Tsytovich et al., 2014, ApJ, 780, 131
(alphabetical order)