IRAS 05170-7156 , the SIMBAD biblio

IRAS 05170-7156 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST08:44:57


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Title First 3 Authors
1987A&AS...70...95D viz 814 193 Warm IRAS sources. I. A catalogue of AGN candidates from the point source catalog. DE GRIJP M.H.K., MILEY G.K. and LUB J.
2000MNRAS.317...55S viz 14       D               1 16418 457 The PSCz catalogue. SAUNDERS W., SUTHERLAND W.J., MADDOX S.J., et al.
2008AJ....136...18W viz 15       D               1 1226 186 Spitzer SAGE survey of the Large Magellanic Cloud. III. Star formation and ∼1000 new candidate young stellar objects. WHITNEY B.A., SEWILO M., INDEBETOUW R., et al.
2009ApJS..184..172G viz 15       D               1 2912 133 High- and intermediate-mass young stellar objects in the Large Magellanic Cloud. GRUENDL R.A. and CHU Y.-H.
2010PASP..122..683K viz 15       D               1 238 89 The SAGE-Spec Spitzer Legacy program: the life cycle of dust and gas in the Large Magellanic Cloud. KEMPER F., WOODS P.M., ANTONIOU V., et al.
2011MNRAS.411.1597W viz 54       D     X         2 230 107 The SAGE-Spec Spitzer Legacy programme: the life-cycle of dust and gas in the Large Magellanic Cloud – point source classification I. WOODS P.M., OLIVEIRA J.M., KEMPER F., et al.
2014AJ....148..124S viz 79           X         2 32 36 Herschel key program Heritage: a far-infrared source catalog for the Magellanic Clouds. SEALE J.P., MEIXNER M., SEWILO M., et al.
2015ApJ...811..145J viz 56       D     X         2 30 12 The dustiest post-main sequence stars in the Magellanic Clouds. JONES O.C., MEIXNER M., SARGENT B.A., et al.
2017MNRAS.470.3250J viz 162           X         4 68 49 The SAGE-Spec Spitzer Legacy program: the life-cycle of dust and gas in the Large Magellanic Cloud. Point source classification - III. JONES O.C., WOODS P.M., KEMPER F., et al.
2020A&A...636A..48G viz 17       D               1 970 ~ The VMC Survey. XXXVII. Pulsation periods of dust-enshrouded AGB stars in the Magellanic Clouds. GROENEWEGEN M.A.T., NANNI A., CIONI M.-R.L., et al.

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