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MGG 9 , the SIMBAD biblio (24 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST15:00:16 |
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 |
---|---|---|---|---|---|---|---|---|---|
2003ApJ...596..240M | 1 | 50 | 158 | Kinematic masses of super-star clusters in M82 from high-resolution near-infrared spectroscopy. | McCRADY N., GILBERT A.M. and GRAHAM J.R. | ||||
2004Natur.428..724P | 13 | 15 | 599 | Formation of massive black holes through runaway collisions in dense young star clusters. | PORTEGIES ZWART S.F., BAUMGARDT H., HUT P., et al. | ||||
2005ApJ...620..238B | 2 | 15 | 128 | Which globular clusters contain intermediate-mass black holes? | BAUMGARDT H., MAKINO J. and HUT P. | ||||
2005ApJ...621..278M | 18 | 47 | Mass segregation and the initial mass function of super star cluster M82-F. | McCRADY N., GRAHAM J.R. and VACCA W.D. | |||||
2005MNRAS.361..311D | 57 | 26 | From young massive star cluster to old globular: the LV-σ0 relationship as a diagnostic tool. | DE GRIJS R., WILKINSON M.I. and TADHUNTER C.N. | |||||
2006A&A...448..881B | 1 | 41 | 101 | Dynamical mass estimates for two luminous star clusters in galactic merger remnants. | BASTIAN N., SAGLIA R.P., GOUDFROOIJ P., et al. | ||||
2006MNRAS.368..121F | 2 | 13 | 62 | Runaway collisions in young star clusters - I. Methods and tests. | FREITAG M., RASIO F.A. and BAUMGARDT H. | ||||
2006MNRAS.368..141F | 20 | 5 | 201 | Runaway collisions in young star clusters - II. Numerical results. | FREITAG M., GURKAN M.A. and RASIO F.A. | ||||
2007ApJ...656..879M | 2 | 14 | 73 | Orbital evolution of an IMBH in the galactic nucleus with a massive central black hole. | MATSUBAYASHI T., MAKINO J. and EBISUZAKI T. | ||||
2007ApJ...663..844M | 59 | 85 | Super star cluster velocity dispersions and virial masses in the M 82 nuclear starburst. | McCRADY N. and GRAHAM J.R. | |||||
2007ApJ...671..349K | 20 | 24 | The ultraluminous X-ray sources near the center of M82. | KONG A.K.H., YANG Y.J., HSIEH P.-Y., et al. | |||||
2008ApJ...684..236C | 38 | X | 1 | 10 | 11 | Gas shepherding by an infalling satellite. | CHANG P. | ||
2008A&A...489.1091M | 35 | 28 | Young star clusters in interacting galaxies - NGC 1487 and NGC 4038/4039. | MENGEL S., LEHNERT M.D., THATTE N.A., et al. | |||||
2009ApJ...691..946M | 115 | X | 3 | 26 | 93 | The sizes and luminosities of massive star clusters. | MURRAY N. | ||
2008AN....329..944M | 23 | 0 | Young star clusters in the Antennae galaxies and NGC 1487. | MENGEL S., LEHNERT M.D., THATTE N., et al. | |||||
2009ApJ...703.1352K | 18 | D | 1 | 39 | 263 | The dynamics of radiation-pressure-dominated H II regions. | KRUMHOLZ M.R. and MATZNER C.D. | ||
2010MNRAS.402.1750G | 92 | D | F | 2 | 31 | 46 | On the velocity dispersion of young star clusters: super-virial or binaries ? | GIELES M., SANA H. and PORTEGIES ZWART S.F. | |
2007ChJAA...7..155D | 75 | C | 1 | 63 | 64 | The Long-term Survival Chances of Young Massive Star Clusters. | DE GRIJS R. and PARMENTIER G. | ||
2011MNRAS.410L...6G | 78 | F | 1 | 43 | 125 | The distinction between star clusters and associations. | GIELES M. and PORTEGIES ZWART S.F. | ||
2010ARA&A..48..431P | 17 | D | 1 | 167 | 902 | Young massive star clusters. | PORTEGIES ZWART S.F., McMILLAN S.L.W. and GIELES M. | ||
2011PASJ...63S.505G | 115 | X F | 2 | 43 | 16 | Diffraction-limited Subaru imaging of M82: Sharp mid-infrared view of the starburst core. | GHANDI P., ISOBE N., BIRKINSHAW M., et al. | ||
2013MNRAS.436.2852B | 16 | D | 1 | 130 | 81 | Constraining globular cluster formation through studies of young massive clusters - I. A lack of ongoing star formation within young clusters. | BASTIAN N., CABRERA-ZIRI I., DAVIES B., et al. | ||
2014MNRAS.437L..21D | 87 | X | 2 | 12 | 211 | Supermassive stars as a source of abundance anomalies of proton-capture elements in globular clusters. | DENISSENKOV P.A. and HARTWICK F.D.A. | ||
2017A&A...597A..28B | 57 | D | X | 2 | 125 | 55 | How can young massive clusters reach their present-day sizes? | BANERJEE S. and KROUPA P. |