J/A+AS/30/261   UBV and Radial Velocities of SMC Supergiants (Ardeberg+, 1977)

Observations of supergiant stars in the Small Magellanic Cloud Ardeberg A., Maurice E. <Astron. Astrophys. Suppl. Ser. 30, 261 (1977)> =1977A&AS...30..261A 1977A&AS...30..261A
ADC_Keywords: Magellanic Clouds ; Stars, supergiant ; Photometry, UBV ; Radial velocities ; MK spectral classification Keywords: Small Magellanic Cloud - supergiant stars - MK classification - radial velocities - UBV photometry Abstract: From observations at the European Southern Observatory, spectrographic and photometric data are presented for 91 supergiant stars belonging to the Small Magellanic Cloud and its Wing. The data include MK classes for 52 stars, radial velocity data for 51 stars and UBV photometry for 90 stars. In V the limiting magnitude for the spectrographic observations is 13.7 and for the photometric observations 13.9. Whenever possible, radial velocities for interstellar CaII and [OII] have been measured and listed. In Remarks to the Catalogue notes are given for the individual stars concerning the obtained data and comparisons with results of previous investigations. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file catalog.dat 100 92 Catalogue notes.dat 80 566 Individual notes -------------------------------------------------------------------------------- See also: V/13 : Probable Members of the SMC (Azzopardi+ 1975, 1979) J/A+A/304/347 : 40 field red supergiants in the SMC (Meliani+, 1995) J/A+A/324/435 : Chemical composition of 6 K supergiants in the SMC (Hill 1997) J/A+AS/142/41 : SMC X-ray sources ROSAT PSPC catalogue (Haberl+, 2000) Byte-by-byte Description of file: catalog.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- [AM77] [1-92] Star sequential number 4- 7 I4 --- HD ? HD (Cat. III/135) number 9- 10 I2 h RAh Right ascension (1975.0) 12- 15 F4.1 min RAm Right ascension (1975.0) 17 A1 --- DE- Declination sign (1975.0) 18- 19 I2 deg DEd Declination (1975.0) 21- 22 I2 arcmin DEm Declination (1975.0) 24- 28 F5.2 mag Vmag ? V magnitude 30- 34 F5.2 mag B-V ? B-V colour index 36- 40 F5.2 mag U-B ? U-B colour index 42- 43 I2 --- NESO ? Number of photometric measurements made with the ESO 1 m telescope 45 I1 --- NBoc ? Number of photometric measurements made with the Bochum-University 61 cm telescope 47- 56 A10 --- SpType MK spectral classification 58 A1 --- Note [*] Remark in notes.dat file 60 I1 --- o_SpType ? Number of spectrograms used for the spectral classification 62- 65 I4 km/s RV ? Stellar radial velocity from absorption-line spectrum 66- 67 A2 --- u_RV [: ] Uncertainty flag on RVs (1) 68 A1 --- n_RV [aeb] Note on RVs (2) 70 A1 --- Note2 [*] Remark in notes.dat file 72 I1 --- o_RV ? Number of spectrograms used for stellar radial velocity determination 74- 77 I4 km/s RVi ? Radial velocity measured for interstellar Ca II from K line 78 A1 --- u_RVi Uncertainty flag on RVi (low-quality measurement) 79 A1 --- Note3 [*] Remark in notes.dat file 81 I1 --- o_RVi ? Number of spectrograms used for interstellar radial velocity determination 83- 86 I4 km/s RVn ? Radial velocity measured for nebular emission lines 87 A1 --- u_RVn Uncertainty flag on RVn (low-quality measurement) 89 A1 --- Note4 [*] Remark in notes.dat file 91 I1 --- o_RVn ? Number of spectrograms used for nebular radial velocity determination 94- 96 I3 --- Sk ? Star number from the catalogues of Sanduleak (1968AJ.....73..246S 1968AJ.....73..246S, 1969AJ.....74..877S 1969AJ.....74..877S) 98-100 A3 --- RMC Star number from the catalogue of Feast et al. (1960MNRAS.121..337F 1960MNRAS.121..337F) -------------------------------------------------------------------------------- Note (1): A colon (:) indicates an uncertainty due to difficulties with the observation or the measurement, or internal standard deviation in the mean velocity (for one spectrogram) larger than 10km/s. A double colon (::) indicates a considerable uncertainty or an internal standard deviation in the mean velocity (for one spectrogram) larger than 15km/s. Note (2): Notes for Stellar radial velocity: a: absorption-line radial velocity, with some information about the emission-line radial velocity given in notes.dat file e: radial velocity calculated also from the emission-line spectrum b: For No 82, RVs= +126(B5), +171(F0) -------------------------------------------------------------------------------- Table 2: Internal standard deviations for single observations of magnitudes and colour indices for programme stars. -------------------------------------------------------------------------------- V 10-11 11-12 12-13 13-14 >14 -------------------------------------------------------------------------------- σV (1m) (n) 0.013 (4) 0.010 (23) 0.011 (24) 0.010 (3) 0.054 (1) σV (60cm) (n) 0.020 (4) 0.016 ( 9) 0.013 ( 6) 0.035 (1) -------------------------------------------------------------------------------- B 10-11 11-12 12-13 13-14 >14 -------------------------------------------------------------------------------- σ(B-V) (1m) (n) 0.010 (5) 0.010 (26) 0.010 (27) 0.008 (3) 0.021 (1) σ(B-V) (60cm)(n) 0.009 (4) 0.010 (11) 0.019 ( 6) -------------------------------------------------------------------------------- U 10-11 11-12 12-13 >13 -------------------------------------------------------------------------------- σ(U-B) (1m) (n) 0.010 (15) 0.011 (29) 0.021 (16) 0.004 (1) σ(U-B) (60cm)(n) 0.015 (10) 0.014 ( 6) 0.024 ( 5) -------------------------------------------------------------------------------- Notes: n indicates number of observations. Unit of σ is magnitude. -------------------------------------------------------------------------------- Byte-by-byte Description of file: notes.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- [AM77] Star number 4- 80 A77 --- Note Text of the note -------------------------------------------------------------------------------- History: Prepared via OCR at CDS. References: Gascoigne, 1954, in Problems of the Magellanic Clouds, The Composition of the Clouds, Australian J. Sci. Suppl., 17, 23 Meinel et al., 1969, Catalogue of Emission Lines in Astrophysical Objects, Universty of Arizona Tucson, Arizona. Schmidt-Kaler, 1965, in Intrinsic Colors and Absolute Magnitudes, Landolt-Boernstein: Numerical Data and Functional Relationships in Science and Technology, Vol. 1, p. 297. Westerlund, 1974, in Proceedings of the First European Astronomical Meeting, Athens, Sept. 4-9, 1972, Vol,. 3, 39
(End) James Marcout, Patricia Bauer [CDS] 29-Mar-2000
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