WR 102ak , the SIMBAD biblio

WR 102ak , the SIMBAD biblio (19 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST20:01:21


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Title First 3 Authors
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.
2005ApJ...623..171R 85 25 Diffuse X-rays from the Arches and Quintuplet clusters. ROCKEFELLER G., FRYER C.L., MELIA F., et al.
2006A&A...458..453V viz 15       D               1 126 78 New Galactic Wolf-Rayet stars, and candidates. An annex to The VIIth Catalogue of Galactic Wolf-Rayet Stars. VAN DER HUCHT K.A.
2008A&A...478..219M 166       D     X         5 36 175 The most massive stars in the Arches cluster. MARTINS F., HILLIER D.J., PAUMARD T., et al.
2010A&A...524A..82L 75             C       2 31 35 The Quintuplet cluster. II. Analysis of the WN stars. LIERMANN A., HAMANN W.-R., OSKINOVA L.M., 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.
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 120           X         3 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               4 123 ~ 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 57       D     X         2 141 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...647A.110G viz 393       D     X         10 29 8 Radio observations of massive stars in the Galactic centre: The Arches Cluster. GALLEGO-CALVENTE A.T., SCHODEL R., ALBERDI A., et al.
2021A&A...649A..43C 167           X C       3 168 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 235       D     X         6 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.
2025A&A...696A..72G 19       D               1 23 ~ Evolution of stars with 60 and 200 M⊙: predictions for WNh stars in the Milky Way. GORMAZ-MATAMALA A.C., ROMAGNOLO A. and BELCZYNSKI K.

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