NAME Pavo I Group , the SIMBAD biblio

NAME Pavo I Group , the SIMBAD biblio (18 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.20CEST00:11:46

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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
1991ApJ...383..467M 139 103 The velocity field of clusters of galaxies within 100 megaparsecs. I. Southern clusters. MOULD J.R., STAVELEY-SMITH L., SCHOMMER R.A., et al.
1992A&A...255...69G 273 68 Groups of galaxies within 80 Mpc. I. Grouping hierarchical method and statistical properties. GOURGOULHON E., CHAMARAUX P. and FOUQUE P.
1992A&AS...93..211F 2164 70 Groups of galaxies within 80 Mpc. II. The catalogue of groups and group members. FOUQUE P., GOURGOULHON E., CHAMARAUX P., et al.
1993A&AS..100...47G viz 4500 387 General study of group membership. II. Determination of nearby groups. GARCIA A.M.
1998MNRAS.296..977B 1 39 136 X-ray spectral analysis of elliptical galaxies from ASCA: the Fe abundance in a multiphase medium. BUOTE D.A. and FABIAN A.C.
1999ApJ...511...34D 1 17 54 The enrichment history of hot gas in poor galaxy groups. DAVIS D.S., MULCHAEY J.S. and MUSHOTZKY R.F.
2000ApJ...543..178G viz 6317 128 Nearby optical galaxies: selection of the sample and identification of groups. GIURICIN G., MARINONI C., CERIANI L., et al.
2000MNRAS.314..375R 246 62 The IRAS PSCz dipole. ROWAN-ROBINSON M., SHARPE J., OLIVER S.J., et al.
2002ApJ...569..720G viz 284 69 Observational mass-to-light ratio of galaxy systems from poor groups to rich clusters. GIRARDI M., MANZATO P., MEZZETTI M., et al.
2004A&A...424.1097S viz 15       D               1 1674 24 Introducing BAX: A database for X-ray clusters and groups of galaxies. SADAT R., BLANCHARD A., KNEIB J.-P., et al.
2006ApJ...653..861M 1         O           60 140 SFI++ I: a new i-band Tully-Fisher template, the cluster peculiar velocity dispersion, and H0. MASTERS K.L., SPRINGOB C.M., HAYNES M.P., et al.
2007MNRAS.374..737F 1 21 43 XMM-Newton study of 0.012 < z < 0.024 groups - I. Overview of the IGM thermodynamics. FINOGUENOV A., PONMAN T.J., OSMOND J.P.F., et al.
2008AJ....135.1738M 16       D               1 33 72 2MTF. I. The Tully-Fisher relation in the two micron all sky survey J, H, and K bands. MASTERS K.L., SPRINGOB C.M. and HUCHRA J.P.
2010ApJ...714.1441S viz 15       D               1 505 17 The linearity of the cosmic expansion field from 300 to 30,000 km/s and the bulk motion of the Local Supercluster with respect to the cosmic microwave background. SANDAGE A., REINDL B. and TAMMANN G.A.
2014MNRAS.439.3666M 55       D     X         2 186 6 The Norma cluster (ACO 3627) - III. The distance and peculiar velocity via the near-infrared Ks-band Fundamental Plane. MUTABAZI T., BLYTH S.L., WOUDT P.A., et al.
2016MNRAS.455.1294D 40           X         1 39 6 HI-deficient galaxies in intermediate-density environments. DENES H., KILBORN V.A., KORIBALSKI B.S., et al.
2021A&A...652A..12K viz 17       D               1 1564 14 The X-CLASS survey: A catalogue of 1646 X-ray-selected galaxy clusters up to z ∼ 1.5. KOULOURIDIS E., CLERC N., SADIBEKOVA T., et al.
2023MNRAS.519..102B 112       D         F     2 35 ~ Calibration of the Tully-Fisher relation in the WISE W1 (3.4 μm) and W2 (4.6 μm) bands. BELL R., SAID K., DAVIS T., et al.

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