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The Mass of M31

Publications of the Astronomical Society of the Pacific, 1981
The projected mass method of Bahcall and Tremaine has been used to derive the mass of the core of M31. From the observed radial velocities of 43 globular clusters, the mass interior to 30' is found to be MI = (9 ± 2) × 1010 Msun. For six clusters with 100' MI = (2.4 ± 1.2) × 1011 Msun. From the observed radial velocities of M32, M33, NGC 147, NGC 185,
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Catalogue of model star clusters in the Milky Way and M31 galaxies

Monthly Notices of the Royal Astronomical Society, 2023
Oleg Y Gnedin   +2 more
exaly  

The Tucana dwarf spheroidal: a distant backsplash galaxy of M31?

Monthly Notices of the Royal Astronomical Society, 2023
Julio Navarro   +2 more
exaly  

First detection and characterization of symbiotic stars in M31

Monthly Notices of the Royal Astronomical Society, 2014
Michael Shara   +2 more
exaly  

M31 satellite masses compared to ΛCDM subhaloes

Monthly Notices of the Royal Astronomical Society, 2014
Erik Tollerud   +2 more
exaly  

Reddening, colour and metallicity of the M31 globular cluster system

Monthly Notices of the Royal Astronomical Society, 2008
Richard De Grijs, De Grijs R
exaly  

Globular clusters in the outer halo of M31: the survey

Monthly Notices of the Royal Astronomical Society, 2008
Rodrigo Ibata   +2 more
exaly  

The ‘remarkable’ M31 globular cluster 037–B327 revisited

Monthly Notices of the Royal Astronomical Society, 2002
Pauline Barmby, Terry Bridges
exaly  

Utilization of waste fish oil and glycerol as carbon sources for polyhydroxyalkanoate production by Salinivibrio sp. M318

International Journal of Biological Macromolecules, 2019
Thuoc Doan, Kumar Sudesh
exaly  

PHOTOGRAPHIC ISOPHOTOMETRY OF M31

Publications of the Astronomical Society of the Pacific, 1970
O. K. Krienke, P. W. Hodge
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