| Show | Sort | Join tables | Column | Constraint | Explain (UCD) |
| | | (ALL) | recno | | Record number assigned by the VizieR team. Should Not be used for identification. (meta.record) (RECORD) |
| | | (1) | IRAS | (char) | IRAS name of object (meta.id) (ID_ALTERNATIVE) |
| | | (1+2+5) | Name | (char) | Alternative identifications of object (meta.id;meta.main) (ID_MAIN) |
| | | (1+2) | Teff | K | Effective temperature (Note 1)
(phys.temperature.effective) (PHYS_TEMP_EFFEC) |
| | | (1) | Dist | pc | (n) Distance (Note 2)
(pos.distance) (PHYS_DISTANCE_TRUE) |
| | | (1) | b_Dist | pc | (n) 16th percentile of distance (Note 2)
(pos.distance) (ERROR) |
| | | (1) | B_Dist | pc | (n) 84th percentile of distance (Note 2)
(pos.distance) (ERROR) |
| | | (1+2) | E(B-V) | mag | (n) Reddening (phot.color.excess) (PHOT_COLOR_EXCESS) |
| | | (1+2) | b_E(B-V) | mag | (n) Lower limit of reddening (phys.absorption;stat.min) (ERROR) |
| | | (1+2) | B_E(B-V) | mag | (n) Upper limit of reddening (phys.absorption;stat.max) (ERROR) |
| | | (1+2) | Lum | Lsun | Luminosity (Note 3)
(phys.luminosity) (PHYS_LUMINOSITY_GENERAL) |
ALL cols | | | |
| | | (1+2) | b_Lum | Lsun | Lower limit of luminosity (Note 3)
(phys.luminosity;stat.min) (ERROR) |
| | | (1+2) | B_Lum | Lsun | Upper limit of luminosity (Note 3)
(phys.luminosity;stat.max) (ERROR) |
| | | (1+2) | LIR | % | IR-to-stellar luminosity ratio (phys.luminosity;arith.ratio) (PHYS_LUMINOSITY_RATIO) |
| | | (1) | SimbadName | (char) | (n)Designation understandable by the Simbad data-base (meta.id) (ID_ALTERNATIVE) |
| | | (1+2+5) | _RA | deg | (i) Right Ascension (J2000) from SIMBAD (not part of the original data) (pos.eq.ra;meta.main) (POS_EQ_RA_MAIN) |
| | | (1+2+5) | _DE | deg | (i) Declination (J2000) from SIMBAD (not part of the original data) (pos.eq.dec;meta.main) (POS_EQ_DEC_MAIN) |
| | | (2+5) | Host | (char) | [SMC LMC] Host Magellanic Cloud (meta.id.parent) (ID_PARENT) |
| | | (2) | Ref | (char) | [a-d] Reference to the paper from which the object was taken (Note 1)
(meta.bib) (REFER_CODE) |
| | | (3+4) | Mi | Msun | Initial mass (phys.mass) (PHYS_MASS_MISC) |
| | | (3+4) | MRLOF | Msun | Mass at the onset of RLOF (phys.mass) (PHYS_MASS_MISC) |
| | | (3+4) | logRRLOF | [Rsun] | Radius at the onset of RLOF (phys.size.radius) (PHYS_SIZE_RADIUS_GENERAL) |
| | | (3+4) | qmin | | Smallest mass ratio in the model grid for this primary model to result in stable mass transfer (phys.mass;meta.modelled) (PHYS_AXIS-RATIO) |
| | | (5) | Porbmean | d | (n) Estimated orbital period determined from its luminosity (Note 1)
(time.period) (TIME_PERIOD) |
ALL cols | | | |
| | | (5) | f_Porbmean | | [0/1] If true (1), the orbital period is a lower limit as the luminosity of the object is larger than the maximum luminosity of the binary models (meta.code) (CODE_MISC) |
| | | (5) | Porbmin | d | (n) Estimated orbital period determined from the lower limit of its luminosity (Note 1)
(time.period) (TIME_PERIOD) |
| | | (5) | Porbmax | d | (n) Estimated orbital period determined from the upper limit of its luminosity (Note 1)
(time.period) (TIME_PERIOD) |
| | | (5) | f_Porbmax | | [0/1] If true (1), the maximum orbital period is a lower limit as the luminosity upper limit of the object is larger than the maximum luminosity of the binary models (meta.code) (CODE_MISC) |
| | | (5) | Agemeansol | yr | Estimated post-mass-transfer age determined from its position in the HRD compared to the solar model grid (time.age) (TIME_AGE) |
| | | (5) | f_Agemeansol | | [0/1] If true (1), the mean post-mass-transfer age is an upper limit, as the luminosity of the object is larger than the maximum luminosity of the solar model grid (meta.code) (CODE_MISC) |
| | | (5) | Ageminsol | yr | Estimated minimum post-mass-transfer age determined from its position in the HRD compared to the solar model grid (time.age;stat.min) (TIME_AGE) |
| | | (5) | f_Ageminsol | | [0/1] If true (1), the minimum post-mass-transfer age is an upper limit, as the luminosity lower limit of the object is larger than the maximum luminosity of the solar model grid (meta.code) (CODE_MISC) |
| | | (5) | Agemaxsol | yr | Estimated maximum post-mass-transfer age determined from its position in the HRD compared to the solar model grid (time.age;stat.max) (TIME_AGE) |
| | | (5) | f_Agemaxsol | | [0/1] If true (1), the maximum post-mass-transfer age is an upper limit, as the luminosity upper limit of the object is larger than the maximum luminosity of the solar model grid (meta.code) (CODE_MISC) |
| | | (5) | Agemeanmp | yr | Estimated post-mass-transfer age determined from its position in the HRD compared to the metal-poor model grid (time.age) (TIME_AGE) |
| | | (5) | f_Agemeanmp | | [0/1] If true (1), the mean post-mass-transfer age is an upper limit, as the luminosity of the object is larger than the maximum luminosity of the metal-poor model grid (meta.code) (CODE_MISC) |
| | | (5) | Ageminmp | yr | Estimated minimum post-mass-transfer age determined from its position in the HRD compared to the metal-poor model grid (time.age;stat.min) (TIME_AGE) |
ALL cols | | | |
| | | (5) | f_Ageminmp | | [0/1] If true (1), the minimum post-mass-transfer age is an upper limit, as the luminosity lower limit of the object is larger than the maximum luminosity of the metal-poor model grid (meta.code) (CODE_MISC) |
| | | (5) | Agemaxmp | yr | Estimated maximum post-mass-transfer age determined from its position in the HRD compared to the metal-poor model grid (time.age;stat.max) (TIME_AGE) |
| | | (5) | f_Agemaxmp | | [0/1] If true (1), the maximum post-mass-transfer age is an upper limit, as the luminosity upper limit of the object is larger than the maximum luminosity of the metal-poor model grid (meta.code) (CODE_MISC) |
ALL cols | | | |