J/MNRAS/496/832    The SDSS/APOGEE catalogue of HgMn stars   (Chojnowski+, 2020)
The SDSS/APOGEE catalogue of HgMn stars.
    Chojnowski S.D., Hubrig S., Hasselquist S., Beaton R.L., Majewski S.R.,
    Garcia-Hernandez D.A., Decolibus D.
   <Mon. Not. R. Astron. Soc., 496, 832-850 (2020)>
   =2020MNRAS.496..832C 2020MNRAS.496..832C    (SIMBAD/NED BibCode)
ADC_Keywords: Stars, peculiar ; Stars, double and multiple ;
              Equivalent widths ; Radial velocities ; Rotational velocities ;
              Spectral types ; Binaries, orbits ; Spectra, infrared
Keywords: stars: chemically peculiar - stars: binaries: spectroscopic -
          stars: rotation
Abstract:
    We report on H-band spectra of chemically peculiar Mercury-Manganese
    (HgMn) stars obtained via the SDSS/APOGEE survey. As opposed to other
    varieties of chemically peculiar stars such as classical Ap/Bp stars,
    HgMn stars lack strong magnetic fields and are defined by extreme
    overabundances of Mn, Hg, and other heavy elements. A satisfactory
    explanation for the abundance patterns remains to be determined, but
    low rotational velocity is a requirement and involvement in
    binary/multiple systems may be as well. The APOGEE HgMn sample
    currently consists of 269 stars that were identified among the
    telluric standard stars as those whose metallic absorption content is
    limited to or dominated by the H-band MnII lines. Due to the fainter
    magnitudes probed by the APOGEE survey as compared to past studies,
    only 9/269 stars in the sample were previously known as HgMn types.
    The 260 newly identified HgMn stars represents a more than doubling of
    the known sample. At least 32 per cent of the APOGEE sample are found
    to be binary or multiple systems, and from multi-epoch spectroscopy,
    we were able to determine orbital solutions for at least one component
    in 32 binaries. Many of the multilined systems include chemically
    peculiar companions, with noteworthy examples being the HgMn+Ap/Bp
    binary HD 5429, the HgMn+HgMn binary HD 298641, and the HgMn+BpMn+Am
    triple system HD 231263. As a further peculiarity, roughly half of the
    sample produces narrow emission in the CI 16895Å line, with widths
    and radial velocities that match those of the MnII lines.
Description:
    The APOGEE instruments are 300-fibre, R=22500, H-band spectrographs
    that operate on the Sloan 2.5m telescope (Gunn et al.
    2006AJ....131.2332G 2006AJ....131.2332G) at Apache Point Observatory (APO, APOGEE-N) and
    on the Du Pont 2.5m telescope (Bowen & Vaughan 1973ApOpt..12.1430B 1973ApOpt..12.1430B) at
    Las Campanas Observatory (LCO, APOGEE-S). Each APOGEE instrument
    records most of the H-band on three detectors, with coverage gaps
    between 15800-15860Å and 16430-16480Å (Wilson et al.
    2019PASP..131e5001W 2019PASP..131e5001W) and with each fibre subtending a ∼2arcsec
    diameter on-sky field of view.
    We also obtained optical spectra of 32 newly discovered HgMn stars, 15
    previously known HgMn stars, and Vega using the Astrophysical Research
    Consortium Echelle Spectrograph (ARCES; Wang et al.
    2003SPIE.4841.1145W 2003SPIE.4841.1145W) on the ARC 3.5m telescope at APO. In each
    exposure, ARCES covers the full optical spectrum (3500-10400Å) at
    a resolution of R=31500.
File Summary:
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 FileName      Lrecl  Records   Explanations
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ReadMe            80        .   This file
table1.dat       152      269   Summary of the APOGEE HgMn sample
table2.dat        42       24   Atomic data for lines detected in the APOGEE
                                spectra of HgMn stars, including the hydrogen
                                Brackett series lines (H-Br)
table3.dat        73     1590   Radial velocity data
table4.dat       132       21   Orbital solutions for SB1s
table5.dat       135       24   Orbital solutions for SB2s and SB3s
table6.dat       116       23   Summary of double-lined and triple-lined
                                spectroscopic binaries
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See also:
  II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)
Byte-by-byte Description of file: table1.dat
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   Bytes Format Units    Label    Explanations
--------------------------------------------------------------------------------
  1-  16 A16    ---      Name     2MASS source identifier (HHMMSSss+DDMMSSs)
 18-  29 A12    ---      OName    Alternative name
 31-  36 F6.3   mag      Hmag     2MASS H-band magnitude
 38-  40 I3     ---      S/N      ? Signal to noise ratio
 42-  43 I2     ---      NRV      Number of radial velocity measurements
 45-  46 I2     ---      Nobs     Number of observed spectra
 48-  49 I2     km/s     vsini    ? Rotational velocity
 51-  52 I2     km/s   e_vsini    ? Error on vsini
 54-  56 I3     10-4nm   EWMnII   ? Average equivalent width of MnII 15413Å
 58-  59 I2     10-4nm   EWCeIII  ? Average equivalent width of CeIII 15961Å
 61-  63 I3     10-4nm   EWCI     ? Average equivalent width of CI 16895Å
 65-  69 F5.1   km/s     RV       ? Average radial velocity
 71-  74 F4.1   km/s   e_RV       ? Error on RV
 76-  80 F5.1   km/s     RVscat   ? Maximum observed radial velocity minus the
                                   minimum observed radial velocity
 82-  85 A4     ---      BinType  Indication of binarity (1)
      87 A1     ---    f_BinType  Flag on BinType (2)
 89-  98 A10    ---      SpType   Spectral type
100- 152 A53    ---    r_SpType   Reference for SpType
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Note (1): Binary type as follows:
    SB1 = Single-lined binary
    SB2 = Double-lined binary
   SB2? = Possible double-lined binary
Note (2): Flag as follows:
    * = An orbital solution is reported in this paper
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Byte-by-byte Description of file: table2.dat
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   Bytes Format Units   Label       Explanations
--------------------------------------------------------------------------------
   1-  6 A6     ---     Ion         Ion name
   8- 16 F9.3   0.1nm   lambda      Vacuum wavelength
  18- 23 F6.3   [-]     loggf       Logarithm of the product of statistical
                                     weight and oscillator strength
  25- 30 F6.3   eV      Elo         Lower state energy
  32- 37 F6.3   eV      Ehi         Upper state energy
  39- 42 F4.2   ---     EW/EW15413  ? Average equivalent width ratio of the
                                     line over MnII 15413Å
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Byte-by-byte Description of file: table3.dat
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   Bytes Format Units   Label Explanations
--------------------------------------------------------------------------------
   1- 16 A16    ---     Name  2MASS source identifier (HHMMSSss+DDMMSSs)
  18- 25 F8.3   d       HJD   Heliocentric Julian date (HJD-245000)
  27- 32 A6     ---     Inst  Instrument (APOGEE or ARCES)
  34- 40 F7.2   km/s    RV1   ? Radial velocity of the primary star
  42- 46 F5.2   km/s  e_RV1   Error on RV1
  48- 54 F7.2   km/s    RV2   ? Radial velocity of the secondary star
  56- 60 F5.2   km/s  e_RV2   ? Error on RV2
  62- 68 F7.2   km/s    RV3   ? Radial velocity of the tertiary star
  70- 73 F4.2   km/s  e_RV3   ? Error on RV3
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Byte-by-byte Description of file: table4.dat
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   Bytes Format Units   Label   Explanations
--------------------------------------------------------------------------------
  1-  16 A16    ---     Name    2MASS source identifier (HHMMSSss+DDMMSSs)
 18-  19 I2     ---     NRV     Number of radial velocity measurements
 21-  27 F7.3   d       P       Orbital period
 29-  33 F5.3   d     e_P       Error on P
 35-  42 F8.3   d       Tmax    Epoch of maximum radial velocity (HJD-245000)
 44-  48 F5.3   d     e_Tmax    Error on Tmax
 50-  54 F5.3   ---     e       Orbital eccentricity
 56-  60 F5.3   ---   e_e       Error on e
 62-  68 F7.3   deg     omega   Argument of the periastron
 70-  74 F5.3   deg   e_omega   Error on omega
 76-  82 F7.3   km/s    gamma   Systemic radial velocity
 84-  88 F5.3   km/s  e_gamma   Error on gamma
 90-  95 F6.3   km/s    K1      Radial velocity semi-amplitude of the primary
                                 star
 97- 101 F5.3   km/s  e_K1      Error on K1
103- 107 F5.3   AU      a1sini  Semimajor axis of the primary star
109- 113 F5.3   AU    e_a1sini  Error on a1sini
115- 119 F5.3   Msun    fM1M2   Mass function
121- 125 F5.3   Msun  e_fM1M2   Error on fM1M2
127- 132 F6.3   ---     chi2    Reduced chi-squared
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Byte-by-byte Description of file: table5.dat
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   Bytes Format Units   Label   Explanations
--------------------------------------------------------------------------------
  1-  17 A17    ---     Name    2MASS source identifier (HHMMSSss+DDMMSSsA)
 19-  20 I2     ---     NRV     Number of radial velocity measurements
 22-  28 F7.3   d       P       ? Orbital period
 30-  34 F5.3   d     e_P       ? Error on P
 36-  43 F8.3   d       Tmax    ? Epoch of maximum radial velocity (HJD-245000)
 45-  49 F5.3   d     e_Tmax    ? Error on Tmax
 51-  55 F5.3   ---     e       ? Orbital eccentricity
 57-  61 F5.3   ---   e_e       ? Error on e
 63-  69 F7.3   deg     omega   ? Argument of the periastron
 71-  76 F6.3   deg   e_omega   ? Error on omega
 78-  84 F7.3   km/s    gamma   ? Systemic radial velocity
 86-  90 F5.3   km/s  e_gamma   ? Error on gamma
 92-  98 F7.3   km/s    K       ? Radial velocity semi-amplitude
100- 104 F5.3   km/s  e_K       ? Error on K
106- 110 F5.3   AU      asini   ? Semimajor axis
112- 116 F5.3   AU    e_asini   ? Error on asini
118- 122 F5.3   Msun    Msini3  ? Dynamical mass
124- 128 F5.3   Msun  e_Msini3  ? Error on Msini3
130- 135 F6.3   ---     chi2    ? Reduced chi-squared
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Byte-by-byte Description of file: table6.dat
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   Bytes Format Units   Label   Explanations
--------------------------------------------------------------------------------
  1-  16 A16    ---     Name    2MASS source identifier (HHMMSSss+DDMMSSs)
 18-  28 A11    ---     Type    Companion type
 30-  34 F5.1   d       P       ? Orbital period
 36-  40 F5.3   ---     M2/M1   ? Mass ratio M2/M1
      42 A1     ---   u_F2/F1   [~] Uncertainty flag on F2/F1
 44-  48 F5.3   ---     F2/F1   ? Flux ratio of MgII 4481Å
 50-  54 F5.3   ---     F2/F12  ? Other value of F2/F1
 56-  57 I2     km/s    vsini1  Rotational velocity of the primary star
 59-  60 I2     km/s  e_vsini1  Error on vsini1
      62 A1     ---   u_vsini2  [~] Uncertainty flag on vsini2
 64-  66 I3     km/s    vsini2  ? Rotational velocity of the secondary star
 68-  69 I2     km/s  e_vsini2  ? Error on vsini2
 71-  72 I2     km/s    vsini3  ? Rotational velocity of the tertiary star
      74 I1     km/s  e_vsini3  ? Error on vsini3
 76- 116 A41    ---     Note    Remarks
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History:
    From electronic version of the journal
(End)                                           Ana Fiallos [CDS]    28-Jun-2023