NAME MW Group , the SIMBAD biblio

NAME MW Group , the SIMBAD biblio (22 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST06:46:40

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2012AJ....144....4M viz 5 119 1400 The observed properties of dwarf galaxies in and around the Local Group. McCONNACHIE A.W.
2013AJ....145..101K viz 15       D               1 872 387 Updated nearby galaxy catalog. KARACHENTSEV I.D., MAKAROV D.I. and KAISINA E.I.
2014A&A...564L...3C viz 1         O           6 20 Globular clusters of NGC 3115 in the near-infrared. Demonstrating the correctness of two opposing scenarios. CANTIELLO M., BLAKESLEE J.P., RAIMONDO G., et al.
2014A&A...565A..98L 1         O           19 68 Chemical composition and constraints on mass loss for globular clusters in dwarf galaxies: WLM and IKN. LARSEN S.S., BRODIE J.P., FORBES D.A., et al.
2014A&A...566A..94K         O           15 16 Feedback by massive stars and the emergence of superbubbles. II. X-ray properties. KRAUSE M., DIEHL R., BOEHRINGER H., et al.
2015AJ....149...54T 39           X         1 156 82 Galaxy groups. TULLY R.B.
2015MNRAS.446.2330S viz 16       D               1 94 29 Overmassive black holes in the MBH-σ diagram do not belong to over (dry) merged galaxies. SAVORGNAN G.A.D. and GRAHAM A.W.
2015A&A...576A..14C viz         O           9 9 VEGAS-SSS. A VST early-type galaxy survey: analysis of small stellar systems. Testing the methodology on the globular cluster system in NGC3115. CANTIELLO M., CAPACCIOLI M., NAPOLITANO N., et al.
2015A&A...579A..33V         O           7 5 Population synthesis of classical low-mass X-ray binaries in the Galactic Bulge. VAN HAAFTEN L.M., NELEMANS G., VOSS R., et al.
2016ApJ...824...42C viz 39           X         1 446 19 Star clusters in M31. VII. Global kinematics and metallicity subpopulations of the globular clusters. CALDWELL N. and ROMANOWSKY A.J.
2016A&A...590A..58M 157           X         4 22 1 Surface term effects on mass estimators. MEMBRADO M. and PACHECO A.F.
2017ApJ...843...16K viz 159           X         4 12390 133 Galaxy groups within 3500 km s–1. KOURKCHI E. and TULLY R.B.
2017A&A...608A..89M viz 40           X         1 75 50 The formation of the Milky Way halo and its dwarf satellites: a NLTE-1D abundance analysis. II. Early chemical enrichment. MASHONKINA L., JABLONKA P., SITNOVA T., et al.
2018A&A...611A..81M 401           X         10 24 ~ Bose-Einstein condensate haloes embedded in dark energy. MEMBRADO M. and PACHECO A.F.
2021MNRAS.502.1623M 42           X         1 14 ~ Spatial segregation impact on star formation in nearby dwarf spheroidal galaxies. MAKAROVA L.N. and MAKAROV D.I.
2022ApJ...926..156D 128           X C       2 14 ~ Improved Lemaitre-Tolman Model and the Mass and Turn-around Radius in Group of Galaxies. II. The Role of Dark Energy. DEL POPOLO A. and CHAN M.H.
2023MNRAS.521..332T 44           X         1 13 1 The cosmic radio background from 150 MHz to 8.4 GHz and its division into AGN and star-forming galaxy flux. TOMPKINS S.A., DRIVER S.P., ROBOTHAM A.S.G., et al.
2023MNRAS.521.3540M 44           X         1 76 4 The LMC impact on the kinematics of the Milky Way satellites: clues from the running solar apex. MAKAROV D., KHOPERSKOV S., MAKAROV D., et al.
2024ApJ...975L..23L 45           X         1 25 ~ Hedgehog: An Isolated Quiescent Dwarf Galaxy at 2.4 Mpc. LI J., GREENE J.E., CARLSTEN S.G., et al.
2025A&A...699A.207M 47           X         1 26 ~ MUSE observations of dwarf galaxies and a stellar stream in the M 83 group. MULLER O., REJKUBA M., FAHRION K., et al.
2025A&A...700A.167T 47           X         1 2 ~ The eROSITA view on the halo mass-temperature relation: From low-mass groups to massive clusters. TOPTUN V., POPESSO P., MARINI I., et al.
2025ApJ...992..106D 93           X         2 46 ~ The HST Legacy Archival Uniform Reduction of Local Group Imaging (LAURELIN). I. Photometry and Star Formation Histories for 36 Ultra-faint Dwarf Galaxies. DURBIN M.J., CHOI Y., SAVINO A., et al.

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