Results 31 to 40 of about 35,587 (387)
The Intrinsic Structure of Sagittarius A* at 1.3 cm and 7 mm [PDF]
Astrophysical Journal, 2021 Sagittarius A* (Sgr A*), the Galactic Center supermassive black hole (SMBH), is one of the best targets in which to resolve the innermost region of an SMBH with very long baseline interferometry (VLBI).
I. Cho +115 more
semanticscholar +1 more source
THE EVENT HORIZON OF SAGITTARIUS A* [PDF]
The Astrophysical Journal, 2009 11 pages, 6 figures, submitted to ...
Broderick, Avery E. +2 more
openaire +5 more sources
The orbit and mass of the Sagittarius dwarf galaxy [PDF]
Monthly Notices of the Royal Astronomical Society, 2000 7 pages, 6 figures, submitted to MNRAS on August 3 ...
Ing‐Guey Jiang, James Binney
openalex +7 more sources
, 2022 Published as part of Boano, Giovanni, Belemsobgo, Urbain, Silvano, Fabrizio, Hema, Emmanuel M., Belemsobgo, Aristide, Dimobe, Kangbéni & Pavia, Marco, 2022, An annotated checklist of the birds of Burkina Faso, pp.
Boano, Giovanni +6 more
openaire +3 more sources
Tango for three: Sagittarius, LMC, and the Milky Way [PDF]
Monthly notices of the Royal Astronomical Society, 2020 We assemble a catalogue of candidate Sagittarius stream members with 5D and 6D phase-space information, using astrometric data from Gaia DR2, distances estimated from RR Lyrae stars, and line-of-sight velocities from various spectroscopic surveys.
E. Vasiliev, V. Belokurov, D. Erkal
semanticscholar +1 more source
A high pitch angle structure in the Sagittarius Arm [PDF]
Astronomy & Astrophysics, 2021 Context. In spiral galaxies, star formation tends to trace features of the spiral pattern, including arms, spurs, feathers, and branches. However, in our own Milky Way, it has been challenging to connect individual star-forming regions to their larger ...
M. Kuhn +8 more
semanticscholar +1 more source
The Sagittarius stream in Gaia Early Data Release 3 and the origin of the bifurcations [PDF]
Astronomy & Astrophysics, 2021 The Sagittarius dwarf spheroidal (Sgr) is a dissolving galaxy being tidally disrupted by the Milky Way (MW). Its stellar stream still poses serious modelling challenges, which hinders our ability to use it effectively as a probe of the MW gravitational ...
P. Ramos +8 more
semanticscholar +1 more source
POLARIZED EMISSION OF SAGITTARIUS A* [PDF]
The Astrophysical Journal, 2009 We explore the parameter space of the two temperature pseudo-Newtonian Keplerian accretion flow model for the millimeter and shorter wavelength emission from Sagittarius A*. A general relativistic ray-tracing code is used to treat the radiative transfer of polarized synchrotron emission from the flow.
Ye-Fei Yuan +8 more
openaire +4 more sources
Ab Initio Horizon-scale Simulations of Magnetically Arrested Accretion in Sagittarius A* Fed by Stellar Winds [PDF]
Astrophysical Journal, 2020 We present 3D general relativistic magnetohydrodynamic (GRMHD) simulations of the accretion flow surrounding Sagittarius A* that are initialized using larger-scale MHD simulations of the ∼30 Wolf–Rayet (WR) stellar winds in the Galactic center.
S. Ressler +3 more
semanticscholar +1 more source
On the orientation of the Sagittarius A* system [PDF]
Astronomy & Astrophysics, 2007 10 pages, 4 figures; Research Note accepted by A&A for ...
Wolfgang J. Duschl +7 more
openaire +3 more sources