[H25] V1 , the SIMBAD biblio

[H25] V1 , the SIMBAD biblio (13 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST06:03:40


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Title First 3 Authors
1925ApJ....62..409H 26 160 NGC 6822, a remote stellar system. HUBBLE E.P.
1967AJ.....72..134K 95 89 Photometry of the nearby irregular galaxy NGC 6822. KAYSER S.E.
1992AJ....104.1374W 427 42 The stellar populations of NGC 6822. WILSON C.D.
1996AJ....112.1928G 1 28 144 The Local Group dwarf galaxy NGC 6822. I. The stellar content. GALLART C., APARICIO A. and VILCHEZ J.M.
2001ApJ...547..765V 1 23 121 First stellar abundances in NGC 6822 from VLT-UVES and Keck-HIRES spectroscopy. VENN K.A., LENNON D.J., KAUFER A., et al.
2002A&A...386..860A 31 11 Variable stars in nearby galaxies. V. Search for Cepheids in field A of NGC 6822. ANTONELLO E., FUGAZZA D., MANTEGAZZA L., et al.
2004AJ....128.2815P viz 126 60 The araucaria project: the distance to the Local Group galaxy NGC 6822 from cepheid variables discovered in a wide-field imaging survey. PIETRZYNSKI G., GIEREN W., UDALSKI A., et al.
2004yCat.2250....0S viz 15       D               3359 107 Combined General Catalogue of Variable Stars. SAMUS N.N. and DURLEVICH O.V.
2006A&A...449..569A 73 1 On the light curve shape of Cepheids in IC 1613 and NGC 6822. ANTONELLO E.
2006ApJ...647.1056G viz 15       D               1 62 56 The Araucaria Project: an accurate distance to the Local Group galaxy NGC 6822 from near-infrared photometry of Cepheid variables. GIEREN W., PIETRZYNSKI G., NALEWAJKO K., et al.
2009ApJ...693..936M 129       D     X         4 25 10 The Cepheid period-luminosity relation (The leavitt law) at mid-infrared wavelengths. III. Cepheids in NGC 6822. MADORE B.F., RIGBY J., FREEDMAN W.L., et al.
2012MNRAS.421.2998F viz 15       D               1 56 20 The Cepheid distance to the Local Group galaxy NGC 6822. FEAST M.W., WHITELOCK P.A., MENZIES J.W., et al.
2014ApJ...794..107R viz 252       D     X C       6 43 12 A new cepheid distance measurement and method for NGC 6822. RICH J.A., PERSSON S.E., FREEDMAN W.L., et al.

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