Ass CMa OB 2 , the SIMBAD biblio

Ass CMa OB 2 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST10:53:40


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Title First 3 Authors
1988A&AS...73...51M 4 4 79 A wide latitude CO survey of the third galactic quadrant. MAY J., MURPHY D.C. and THADDEUS P.
1997A&A...327..325M viz 174 47 Physical properties of molecular clouds in the southern outer Galaxy. MAY J., ALVAREZ H. and BRONFMAN L.
1998AJ....115.1958T 61 20 Galactic clusters with associated cepheid variables. VI. Anonymous van den Bergh (C0634+031) and CV Monocerotis. TURNER D.G., PEDREROS M.H. and WALKER A.R.
2000MNRAS.318.1023K 163 8 The region of Collinder 121. KALTCHEVA N.T.
2003MNRAS.346.1143B viz 153 17 On the nature of Collinder 121: insights from the low-mass pre-main sequence. BURNINGHAM B., NAYLOR T., JEFFRIES R.D., et al.
2005AJ....130.1805D viz 149 40 The young cluster NGC 2362. DAHM S.E.
2007A&A...470..685L 15       D               2 214 151 Searching for links between magnetic fields and stellar evolution. II. The evolution of magnetic fields as revealed by observations of Ap stars in open clusters and associations. LANDSTREET J.D., BAGNULO S., ANDRETTA V., et al.
2008A&A...477..917P viz 15       D               1 179 41 β Cephei stars in the ASAS-3 data. II. 103 new β Cephei stars and a discussion of low-frequency modes. PIGULSKI A. and POJMANSKI G.
2010A&A...521A..39O viz 38           X         1 158 4 A revisit to the region of Collinder 132 using Carte du Ciel and Astrographic Catalogue plates. ORELLANA R.B., DE BIASI M.S., BUSTOS FIERRO I.H., et al.
2011ApJ...726...81A 40           X         1 18 92 Constraints on the cosmic-ray density gradient beyond the solar circle from Fermi γ-ray observations of the third galactic quadrant. ACKERMANN M., AJELLO M., BALDINI L., et al.
2023MNRAS.523.5306F 435   K A D     X   F     10 46 ~ Stellar clustering and the kinematics of stars around Collinder 121 using Gaia DR3. FLEMING G.D., KIRK J.M. and WARD-THOMPSON D.
2024Natur.631...49S viz 45           X         1 62 ~ Most nearby young star clusters formed in three massive complexes. SWIGGUM C., ALVES J., BENJAMIN R., et al.

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