AzV 435 , the SIMBAD biblio

AzV 435 , the SIMBAD biblio (22 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST09:55:00


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Title First 3 Authors
1982A&AS...50..291A 523 98 Catalogue of the Small Magellanic Cloud star members. AZZOPARDI M. and VIGNEAU J.
1995ApJ...438..188M 308 381 Massive stars in the field and associations of the Magellanic Clouds : the upper mass limit, the initial mass function and a critical test of main-sequence stellar evolutionary theory. MASSEY P., LANG C.C., DE GIOIA-EASTWOOD K., et al.
2002ApJS..141...81M viz 1417 322 A UBVR CCD survey of the Magellanic clouds. MASSEY P.
2004AJ....127.1632O viz 1516 61 Massive field stars and the stellar clustering law. OEY M.S., KING N.L. and PARKER J.W.
2005ApJ...627..477M 1 52 168 The physical properties and effective temperature scale of O-type stars as a function of metallicity. II. Analysis of 20 more Magellanic cloud stars and results from the complete sample. MASSEY P., PULS J., PAULDRACH A.W.A., et al.
2007A&A...473..603M 15       D               1 123 294 The empirical metallicity dependence of the mass-loss rate of O- and early B-type stars. MOKIEM M.R., DE KOTER A., VINK J.S., et al.
2008A&A...477..223Y 15       D               1 66 111 On the evolution and fate of super-massive stars. YUNGELSON L.R., VAN DEN HEUVEL E.P.J., VINK JORICK S., et al.
2009PASP..121..634B viz 15       D               1 288 10 The Far Ultraviolet Spectroscopic Explorer legacy in the Magellanic Clouds: an online stellar sight line atlas. BLAIR W.P., OLIVEIRA C., LAMASSA S., et al.
2009ApJ...700..844P viz 15       D               2 319 28 A FUSE survey of the rotation rates of very massive stars in the Small and Large Magellanic Clouds. PENNY L.R. and GIES D.R.
2010AJ....140..416B viz 15       D               1 5310 140 Spitzer SAGE-SMC infrared photometry of massive stars in the Small Magellanic Cloud. BONANOS A.Z., LENNON D.J., KOHLINGER F., et al.
2012ApJ...745..173W viz 92       D       C       2 307 56 Interstellar H I and H2 in the Magellanic Clouds: an expanded sample based on ultraviolet absorption-line data. WELTY D.E., XUE R. and WONG T.
2012ApJ...753..173E 114           X C       2 23 8 A rare early-type star revealed in the wing of the Small Magellanic Cloud. EVANS C.J., HAINICH R., OSKINOVA L.M., et al.
2012A&A...543A..95R 397       D     X C F     9 26 33 Nitrogen line spectroscopy in O-stars. III. The earliest O-stars. RIVERO GONZALEZ J.G., PULS J., MASSEY P., et al.
2012ApJS..202...17S viz 15       D               1 30 2 A detailed far-ultraviolet spectral atlas of O-type stars. SMITH M.A.
2015ApJ...811...78T viz 16       D               1 90 46 Elemental depletions in the Magellanic Clouds and the evolution of depletions with metallicity. TCHERNYSHYOV K., MEIXNER M., SEALE J., et al.
2017MNRAS.470.3765M viz 175       D     X         5 109 2 Mass-loss rates from mid-infrared excesses in LMC and SMC O stars. MASSA D., FULLERTON A.W. and PRINJA R.K.
2022ApJ...936..112D viz 17       D               1 1353 3 Classical OBe Stars as Post-supernova Runaways: Confirming Binary Origins. DALLAS M.M., OEY M.S. and CASTRO N.
2023A&A...675A.154V viz 17       D               1 256 ~ X-Shooting ULLYSES: Massive stars at low metallicity I. Project description. VINK J.S., MEHNER A., CROWTHER P.A., et al.
2023MNRAS.525.2820K 192       D       C F     2 95 ~ Cold diffuse interstellar medium of Magellanic Clouds: I. HD molecule and cosmic-ray ionization rate. KOSENKO D.N. and BALASHEV S.A.
2025A&A...695A.198B viz 112       D     X         3 247 ~ X-Shooting ULLYSES: Massive stars at low metallicity XI. Pipeline-determined physical properties of Magellanic Cloud OB stars. BESTENLEHNER J.M., CROWTHER P.A., HAWCROFT C., et al.
2025A&A...696L..16B 19       D               1 38 ~ First detections of CO absorption in the Magellanic Clouds and direct measurement of the CO-to-H2 ratio. BALASHEV S.A., KOSENKO D.N. and NOTERDAEME P.
2025AJ....170..176T 19       D               3 60 ~ An Ultraviolet Study of CO Chemistry in the Magellanic Clouds. TCHERNYSHYOV K., WERK J.K. and ROMAN-DUVAL J.

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