Cl Alessi 95 , the SIMBAD biblio

Cl Alessi 95 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST18:23:02


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Title First 3 Authors
2012MNRAS.421.1040M                   Z 1 56 3 A cluster of class I/f/II young stellar objects discovered near the Cepheid SU Cas. MAJAESS D., TURNER D.G. and GIEREN W.
2012MNRAS.422.2501T 1416 T K A S   X C       34 69 20
Alessi 95 and the short-period cepheid SU Cassiopeiae.
TURNER D.G., MAJAESS D.J., LANE D.J., et al.
2012ApJ...753..144M 487     A S   X C       11 16 10 Anchoring the distance scale via X-Ray/Infrared data for cepheid clusters: SU Cas. MAJAESS D., TURNER D.G., GALLO L., et al.
2013A&A...550A..70G viz 16       D               1 201 45 Baade-Wesselink distances to Galactic and Magellanic Cloud Cepheids and the effect of metallicity. GROENEWEGEN M.A.T.
2013A&A...560A..22M 39           X         1 23 13 Anchors for the cosmic distance scale: the Cepheids U Sagittarii, CF Cassiopeiae, and CEab Cassiopeiae. MAJAESS D., CARRARO G., MONI BIDIN C., et al.
2013AstL...39..634U 3 2 Spectroscopic studies of the small-amplitude Cepheid SU Cas. USENKO I.A., KLOCHKOVA V.G. and TAVOLZHANSKAYA N.S.
2017MNRAS.464.1119C 57       D     X         2 63 10 New open cluster Cepheids in the VVV survey tightly constrain near-infrared period-luminosity relations. CHEN X., DE GRIJS R. and DENG L.
2018ApJ...854...79L 16       D               1 11 1 A color-locus method for mapping RV using ensembles of stars. LEE A., GREEN G.M., SCHLAFLY E.F., et al.
2018A&A...616A.112S viz 99       D       C       2 79 11 Deep secrets of intermediate-mass giants and supergiants. Models with rotation seem to overestimate mixing effects on the surface abundances of C, N, and Na. SMILJANIC R., DONATI P., BRAGAGLIA A., et al.
2018AJ....156..171L viz 41           X         1 438 53 Cepheid abundances: multiphase results and spatial gradients. LUCK R.E.
2022A&A...668A..13H viz 152       D     X C       3 87 3 Open clusters housing classical Cepheids in Gaia DR3. HAO C.J., XU Y., WU Z.Y., et al.

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