IRAS Z05259-7052 , the SIMBAD biblio

IRAS Z05259-7052 , the SIMBAD biblio (15 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST16:24:42


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Title First 3 Authors
2008AJ....136.1242F viz 15       D               1 47759 44 The properties of long-period variables in the Large Magellanic Cloud from MACHO. FRASER O.J., HAWLEY S.L. and COOK K.H.
2009ApJS..184..172G viz 15       D               2 2912 133 High- and intermediate-mass young stellar objects in the Large Magellanic Cloud. GRUENDL R.A. and CHU Y.-H.
2009AcA....59..239S viz 15       D               1 92001 185 The Optical Gravitational Lensing Experiment. The OGLE-III catalog of variable stars. IV. Long-period variables in the Large Magellanic Cloud. SOSZYNSKI I., UDALSKI A., SZYMANSKI M.K., et al.
2011ApJ...735..127V 55 38 Discovery and analysis of 21 µm feature sources in the Magellanic clouds. VOLK K., HRIVNAK B.J., MATSUURA M., et al.
2011A&A...530A..90V viz 15       D               1 1414 46 The optically bright post-AGB population of the LMC. VAN AARLE E., VAN WINCKEL H., LLOYD EVANS T., et al.
2011A&A...536A..60S viz 15       D               1 43415 15 Long period variables in the Large Magellanic Cloud from the EROS-2 survey. SPANO M., MOWLAVI N., EYER L., et al.
2014MNRAS.439.1472M 596       D     X C F     14 51 37 Spitzer Space Telescope spectra of post-AGB stars in the Large Magellanic Cloud - polycyclic aromatic hydrocarbons at low metallicities. MATSUURA M., BERNARD-SALAS J., LLOYD EVANS T., et al.
2014ApJ...791...28S 286       D     X         8 72 48 Carbon-rich dust past the asymptotic giant branch: aliphatics, aromatics, and fullerenes in the Magellanic Clouds. SLOAN G.C., LAGADEC E., ZIJLSTRA A.A., et al.
2015ApJ...805...78H 367       D     X         10 32 3 Variability in proto-planetary nebulae. III. Light curve studies of Magellanic Cloud carbon-rich objects. HRIVNAK B.J., LU W., VOLK K., et al.
2015MNRAS.454.1468K viz 250       D     X         7 2116 79 Optically visible post-AGB stars, post-RGB stars and young stellar objects in the Large Magellanic Cloud. KAMATH D., WOOD P.R. and VAN WINCKEL H.
2016MNRAS.462.1551Y 16       D               1 29 6 On the aliphatic versus aromatic content of the carriers of the 'unidentified' infrared emission features. YANG X.J., GLASER R., LI A., et al.
2019A&A...626A..92G viz 138       D     X C       3 225 ~ 30-micron sources in galaxies with different metallicities. GLADKOWSKI M., SZCZERBA R., SLOAN G.C., et al.
2020A&A...637A..82D 16       D               1 19 ~ Mechanochemical synthesis of aromatic infrared band carriers. The top-down chemistry of interstellar carbonaceous dust grain analogues. DARTOIS E., CHARON E., ENGRAND C., et al.
2020A&A...641A.142S viz 16       D   O           2 20 ~ Validating post-AGB candidates in the LMC and SMC using SALT spectra. SZCZERBA R., HAJDUK M., PAVLENKO Y.V., et al.
2022A&A...665A.153J 17       D               2 67 2 The mid-infrared aliphatic bands associated with complex hydrocarbons. JENSEN P.A., SHANNON M.J., PEETERS E., et al.

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