SK 183 , the SIMBAD biblio

SK 183 , the SIMBAD biblio (23 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST07:50:14


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Title First 3 Authors
1969AJ.....74..877S 48 71 Proven and probable members in the Wing of the Small Magellanic Cloud. SANDULEAK N.
1976A&AS...24..357S 315 50 Starlight polarization in the Magellanic Cloud regions. SCHMIDT T.
1978A&AS...33..193I 104 25 Lichtelektrische Photometrie in der Kleinen Magellanschen Wolke. ISSERSTEDT J.
1991AJ....101..933H 14 13 A study of the young massive cluster N 90 in the SMC. HUTCHINGS J.B., THOMPSON I.B., CARTLEDGE S., 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.
2012ApJ...748...64G 38           X         1 29 19 The clustered nature of star formation. Pre-main-sequence clusters in the star-forming region NGC 602/N90 in the Small Magellanic Cloud. GOULIERMIS D.A., SCHMEJA S., DOLPHIN A.E., et al.
2012ApJ...753..173E 2197   K A S   X C       56 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.
2013ApJ...765...73O 269           X         7 31 7 Discovery of X-ray emission from young suns in the Small Magellanic Cloud. OSKINOVA L.M., SUN W., EVANS C.J., et al.
2017A&A...601A..79S viz 79           X         2 99 40 The VLT-FLAMES Tarantula Survey. XXVI. Properties of the O-dwarf population in 30 Doradus. SABIN-SANJULIAN C., SIMON-DIAZ S., HERRERO A., et al.
2017ApJ...846..110D 119           X         3 21 4 Photometric determination of the mass accretion rates of pre-main-sequence stars. V. Recent star formation in the 30 Dor nebula. DE MARCHI G., PANAGIA N. and BECCARI G.
2018A&A...609A..94H 241           X C       5 36 11 Observational properties of massive black hole binary progenitors. HAINICH R., OSKINOVA L.M., SHENAR T., et al.
2019A&A...625A.104R viz 179       D     X         5 347 72 Testing massive star evolution, star formation history, and feedback at low metallicity. Spectroscopic analysis of OB stars in the SMC Wing. RAMACHANDRAN V., HAMANN W.-R., OSKINOVA L.M., et al.
2019A&A...629A..91Y viz 16       D               1 1374 29 Evolved massive stars at low-metallicity. I. A source catalog for the Small Magellanic Cloud. YANG M., BONANOS A.Z., JIANG B.-W., et al.
2021A&A...646A.106S 43           X         1 10 12 A dearth of young and bright massive stars in the Small Magellanic Cloud. SCHOOTEMEIJER A., LANGER N., LENNON D., et al.
2022ApJ...936..112D viz 17       D               2 1353 3 Classical OBe Stars as Post-supernova Runaways: Confirming Binary Origins. DALLAS M.M., OEY M.S. and CASTRO N.
2022ApJ...938...82O viz 766           X C       17 44 1 Sequential Star Formation in the Young SMC Region NGC 602: Insights from ALMA. O'NEILL T.J., INDEBETOUW R., SANDSTROM K., et al.
2022A&A...666A.189R 43           X         1 28 6 Stellar wind properties of the nearly complete sample of O stars in the low metallicity young star cluster NGC 346 in the SMC galaxy. RICKARD M.J., HAINICH R., HAMANN W.-R., et al.
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.
2024ApJ...975...18Z 45           X         1 10 ~ Discovering Subsolar Metallicity Brown Dwarf Candidates in the Small Magellanic Cloud. ZEIDLER P., SABBI E., NOTA A., et al.
2025A&A...695A.198B viz 19       D               1 247 ~ 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...697A.114P viz 19       D               1 198 ~ New empirical mass-loss recipe for UV radiation line-driven winds of hot stars across various metallicities. PAULI D., OSKINOVA L.M., HAMANN W.-R., et al.
2025AJ....170..262M 1120           X C       23 10 ~ Detection of a Deeply Embedded Protocluster Candidate in NGC 602 with JWST. MEENA B., ZEIDLER P., SABBI E., et al.

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