[BHE2002] WLM 1 , the SIMBAD biblio

[BHE2002] WLM 1 , the SIMBAD biblio (23 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST09:38:25

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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
1985AJ.....90.1464S 73 77 The brightest stars in nearby galaxies. VI. Cepheids and the brightest stars in WLM. SANDAGE A. and CARLSON G.
1997AJ....114..147M 40 60 Stellar populations of the dwarf irregular galaxy WLM. MINNITI D. and ZIJLSTRA A.A.
1999ApJ...521..577H viz 1 8 40 Hubble space Telescope Studies of the WLM galaxy. I. The age and metallicity of the globular cluster. HODGE P.W., DOLPHIN A.E., SMITH T.R., et al.
2000A&A...358..471F 127 39 The elliptical galaxy formerly known as the Local Group: merging the globular cluster systems. FORBES D.A., MASTERS K.L., MINNITI D., et al.
2000ApJ...531..804D 8 3 77 Hubble space telescope studies of the WLM galaxy. II. The star formation history from field stars. DOLPHIN A.E.
2002AJ....123.1454B 100 117 Compact star clusters in nearby dwarf irregular galaxies. BILLETT O.H., HUNTER D.A. and ELMEGREEN B.G.
2002AJ....124..896S 9 24 The oldest stars of the extremely metal-poor local group dwarf irregular galaxy Leo A. SCHULTE-LADBECK R.E., HOPP U., DROZDOVSKY I.O., et al.
2004ApJ...614L.109G 1 9 34 Surface brightness and stellar populations at the outer edge of the Large Magellanic Cloud: no stellar halo yet. GALLART C., STETSON P.B., HARDY E., et al.
2006AJ....131.1426S 12 8 WLM-1: an old, nonrotating, gravitationally unperturbed, highly elliptical extragalactic globular cluster. STEPHENS A.W., CATELAN M. and CONTRERAS R.P.
2006MNRAS.368.1443M 22 26 A `super' star cluster grown old: the most massive star cluster in the Local Group. MA J., DE GRIJS R., YANG Y., et al.
2007A&A...466..501V viz 74             C       1 11 11 Carbon stars and C/M ratio in the WLM dwarf irregular galaxy. VALCHEVA A.T., IVANOV V.D., OVCHAROV E.P., et al.
2009AJ....137.4361D 112           X         3 55 33 Scl-dE1 GC1: an extended globular cluster in a low-luminosity dwarf elliptical galaxy. DA COSTA G.S., GREBEL E.K., JERJEN H., et al.
2009ApJ...699....1L 37           X         1 93 22 Stellar metallicities and kinematics in a gas-rich dwarf galaxy: first calcium triplet spectroscopy of red giant branch stars in WLM. LEAMAN R., COLE A.A., VENN K.A., et al.
2008A&ARv..15..289T viz 15       D               1 299 47 The expansion field: the value of H0. TAMMANN G.A., SANDAGE A. and REINDL B.
2011A&A...532A.104N viz 15       D               1 976 78 Hubble flow around Fornax cluster of galaxies. NASONOVA O.G., DE FREITAS PACHECO J.A. and KARACHENTSEV I.D.
2012MNRAS.423.3589W 38           X         1 41 5 Collisionless dynamics in globular clusters. WILLIAMS L.L.R., BARNES E.I. and HJORTH J.
2013MNRAS.435..809A 38           X         1 16 11 Mergers of multimetallic globular clusters: the role of dynamics. AMARO-SEOANE P., KONSTANTINIDIS S., BREM P., et al.
2014A&A...565A..98L 3947 T K A D S O X C       100 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.
2014ApJ...797...15L viz 40           X         1 18 52 Nitrogen abundances and multiple stellar populations in the globular clusters of the Fornax dSph. LARSEN S.S., BRODIE J.P., GRUNDAHL F., et al.
2015AJ....149..132B 94       D     X         3 177 4 Hubble Space Telescope snapshot search for planetary nebulae in globular clusters of the Local Group. BOND H.E.
2022A&A...660A..88L viz 17       D               14 80 13 The chemical composition of globular clusters in the Local Group. LARSEN S.S., EITNER P., MAGG E., et al.
2023MNRAS.521.3847S 810     A S   X C F     16 19 ~ The properties of RR Lyrae variable stars in the isolated Local Group dwarf galaxy WLM. SARAJEDINI A.
2023RNAAS...7...23W 331     A     X         8 3 ~ The JWST Resolved Stellar Populations Early Release Science Program. III. Photometric Star-Galaxy Separations for NIRCam. WARFIELD J.T., RICHSTEIN H., KALLIVAYALIL N., et al.

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