Details on Acronym: N206-FS
N206-FS (N 206 FLAMES Survey) ***** Avoid the usage of N206-FS, prefer [RHH2018] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym: [RHH2018]
[RHH2018] (Ramachandran+Hainich+Hamann+, 2018)= (N206-FS) Write:<<[RHH2018] NNN>>
<<[RHH2018] NNNa>> N: 234+4 Object:OB* + WR binary + ? (SIMBAD class: Star) Note:VLT FLAMES observations of N=234 spectra in the LMC superbubble LHA 120-N 206.
The whole sample encompasses the spectra of 164 OB stars (including 9 Of stars), 17 A-type stars, 2 WR binaries, 2 candidate high mass X-ray binary (HMXB) positions, 32 fiber positions in the HII region, 8 fiber positions in the X-ray superbubble, 9 fiber positions in the SNR.
2018A&A...609A...7R (Paper I): N=9 Of stars (including two binaries, hence the additional format(NNNa)
2018A&A...615A..40R (Paper II): N=155 other OB-type stars + N=2 WR binaries
Use of archival HST, IUE, FUSE data. in source:Magellanic Clouds:LMC:LHA 120-N 206 = LHA 120-N 206 Ref:=2018A&A...609A...7R byRAMACHANDRAN V. , HAINICH R., HAMANN W.-R., OSKINOVA L.M., SHENAR T., SANDER A.A.C., TODT H., GALLAGHER J.S. Astron. Astrophys., 609A, 7-7 (2018) Stellar population of the superbubble N 206 in the LMC. I. Analysis of the Of-type stars. oN206-FS 186 not yet identified in SIMBAD. oFig. 1, Table 1: <[RHH2018] NNN> N=9 among (Nos 66-214). Table 3: <[RHH2018] NNNa> (Nos 131a-131b, 180a-180b). Ref:=2018A&A...615A..40R byRAMACHANDRAN V. , HAMANN W.-R., HAINICH R., OSKINOVA L.M., SHENAR T., SANDER A.A.C., TODT H., GALLAGHER J.S. Astron. Astrophys., 615A, 40-40 (2018) Stellar population of the superbubble N 206 in the LMC. II. Parameters of the OB and WR stars, and the total massive star feedback. oTables 1, 3-4, A.1-A.3: <[RHH2018] NNN> N=155+2 among (Nos 1-234). =E=Catalogue in electronic form as <J/A+A/609/A7/> =E=Catalogue in electronic form as <J/A+A/615/A40/> Originof the Acronym: S = Created by Simbad, the CDS Database
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