[BSP2001] 8 , the SIMBAD biblio

[BSP2001] 8 , the SIMBAD biblio (22 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST23:44:01

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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
1996ApJ...461..750C 1 45 185 The discovery of hot stars near the Galactic center thermal radio filaments. COTERA A.S., ERICKSON E.F., COLGAN S.W.J., et al.
2001AJ....122.1875B 48 48 2 micron narrowband adaptive optics imaging in the Arches cluster. BLUM R.D., SCHAERER D., PASQUALI A., et al.
2002ApJ...581..258F viz 220 283 Massive stars in the Arches Cluster. FIGER D.F., NAJARRO F., GILMORE D., et al.
2004ApJ...611L.105N 2 13 99 Metallicity in the galactic center: the Arches cluster. NAJARRO F., FIGER D.F., HILLIER D.J., et al.
2005ApJ...623..171R 85 25 Diffuse X-rays from the Arches and Quintuplet clusters. ROCKEFELLER G., FRYER C.L., MELIA F., et al.
2008A&A...478..219M 91       D     X         3 36 175 The most massive stars in the Arches cluster. MARTINS F., HILLIER D.J., PAUMARD T., et al.
2010A&A...516A..35H 38           X         1 28 23 Obscured clusters. III. Follow-up observations of Mercer 23. HANSON M.M., KURTEV R., BORISSOVA J., et al.
2010MNRAS.408..731C 43           X         1 41 437 The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150M☉ stellar mass limit. CROWTHER P.A., SCHNURR O., HIRSCHI R., et al.
2011MNRAS.417..114D viz 15       D               1 184 58 Hubble Space Telescope Paschen α survey of the Galactic Centre: data reduction and products. DONG H., WANG Q.D., COTERA A., et al.
2011A&A...535A..56G 16       D               1 36 132 The Eddington factor as the key to understand the winds of the most massive stars. Evidence for a Γ-dependence of Wolf-Rayet type mass loss. GRAEFENER G., VINK J.S., DE KOTER A., et al.
2012ApJ...751L..34V 16       D               1 24 62 The transition mass-loss rate: calibrating the role of line-driven winds in massive star evolution. VINK J.S. and GRAFENER G.
2012MNRAS.425..884D 15       D               1 200 21 A multiwavelength study of evolved massive stars in the Galactic Centre. DONG H., WANG Q.D. and MORRIS M.R.
2014A&A...569A..20M viz 39           X         1 51 8 Massive stars in the giant molecular cloud G23.3-0.3 and W41. MESSINEO M., MENTEN K.M., FIGER D.F., et al.
2015MNRAS.446..842D 234           X C       5 46 8 Origins of massive field stars in the Galactic Centre: a spectroscopic study. DONG H., MAUERHAN J., MORRIS M.R., et al.
2015ApJ...805..110M 78           X         2 116 16 Massive stars in the W33 giant molecular complex. MESSINEO M., CLARK J.S., FIGER D.F., et al.
2018A&A...617A..65C viz 16       D               1 225 9 The Arches cluster revisited. I. Data presentation and stellar census. CLARK J.S., LOHR M.E., NAJARRO F., et al.
2018A&A...617A..66L viz 80           X         2 27 9 The Arches cluster revisited. II. A massive eclipsing spectroscopic binary in the Arches cluster. LOHR M.E., CLARK J.S., NAJARRO F., et al.
2018MNRAS.480.1507T viz 16       D               2 123 ~ The 1.87- and 2.07-µm observations of three Galactic Centre clusters with miniTAO at Atacama: classification of stellar components in massive star clusters. TANAKA M., OKUMURA S.-I., TAKAHASHI H., et al.
2019A&A...623A..84C viz 41           X         1 141 1 The Arches cluster revisited. III. An addendum to the stellar census. CLARK J.S., LOHR M.E., PATRICK L.R., et al.
2021A&A...649A..43C 42           X         1 168 11 Constraining the population of isolated massive stars within the Central Molecular Zone. CLARK J.S., PATRICK L.R., NAJARRO F., et al.
2023MNRAS.521.4473C 1019       D S   X C F     21 91 ~ The Arches cluster revisited - IV. Observational constraints on the binary properties of very massive stars. CLARK J.S., LOHR M.E., NAJARRO F., et al.
2024A&A...692A..23C 152       D     X         4 29 ~ A multi-frequency, multi-epoch radio continuum study of the Arches cluster with the Very Large Array. CANO-GONZALEZ M., SCHODEL R., ALBERDI A., et al.

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