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J/A+AS/104/315      Member of Herbig Ae/Be stellar group     (The+ 1994)
A new catalogue of members and candidate members of the Herbig Ae/Be (HAEBE)
stellar group
     The P.S., de Winter D., Perez M.R.
    <Astron. Astrophys. Suppl. Ser. 104, 315 (1994)>
    =1994A&AS..104..315T      (SIMBAD/NED RefCode)
ADC_Keywords: Stars, Be ;

Keywords: catalogs - stars: Be - stars: formation - stars: pre-main sequence -
          infrared: stars

Description:
    An up-to-date catalogue of Herbig Ae/Be (HAEBE) stars and related
    objects is listed in five tables, containing 287 objects. Table 1
    contains all Ae and Be stars which historically are recognized as true
    HAEBE stars or potential candidate members. Table 2 gives the stars of
    spectral type Fe, and emission line stars with very uncertain or
    unknown spectral type. In Table 3 are given all known Extreme Emission
    Line Objects (EELOs), of which most have not been identified to belong
    to any specific group. Table 4a and b list other Bep or B[e] stars
    with strong IR-excess and unknown spectral type. Table 5 contains the
    non-emission line possible young objects. Furthermore, Table 6
    contains 35 stars rejected from former published lists of HAEBE stars.
    In these tables we are including coordinates, spectral types, visual
    magnitudes, ranges in photometric variability and references of
    several key publications related to each object. Relevant remarks,
    such as the presence of a nebula in the vicinity of an object, are
    also given.

File Summary:

       FileName      Lrecl  Records   Explanations

ReadMe            80        .   This file
liste2.txt        64       79   Abbreviations of the objects designations
liste3.dat        75       31   Stars of which the optical and IRAS coordinates
                               are offsetted by ≥ 30"
table1.dat       284      108   Herbig Ae/Be members and candidate members
table2.dat       284       23   F-type PMS stars, potential candidates and
                               those with unknown spectral type
table3.dat       284       23   Extreme emission line objects (EELOs)
table4a.dat      284       32   Other early type emission line stars with
                               IR-excess from AIS
table4b.dat      284       87   Other early type emission line stars with
                               IR-excess from DoH
table5.dat       284       14   Non-emission line early type shell stars and
                               young stellar candidates
table6.dat       284       35   Emission line stars rejected as Herbig Ae/Be
                               candidates


Byte-by-byte Description of file: liste3.dat

   Bytes Format  Units   Label    Explanations

   1- 15  A15    ---     Name     Optical source name
  16- 17  I2     h       RAh      Right ascension 1950
  19- 20  I2     min     RAm      Right ascension 1950
  22- 25  F4.1   s       RAs      Right ascension 1950
      28  A1     ---     DE-      Declination sign
  29- 30  I2     deg     DEd      Declination 1950
  32- 33  I2     arcmin  DEm      Declination 1950
  35- 38  F4.1   arcsec  DEs      Declination 1950
  40- 54  A15    ---     IRAS     IRAS source
  56- 57  I2     h      RA.IRASh  Right ascension 1950 from IRAS
  59- 60  I2     min    RA.IRASm  Right ascension 1950 from IRAS
  62- 65  F4.1   s      RA.IRASs  Right ascension 1950 from IRAS
      67  A1     ---    DE.IRAS-  Declination sign from IRAS
  68- 69  I2     deg    DE.IRASd  Declination 1950 from IRAS
  71- 72  I2     arcmin DE.IRASm  Declination 1950 from IRAS
  74- 75  I2     arcsec DE.IRASs  Declination 1950 from IRAS


Byte-by-byte Description of file: table*.dat

   Bytes Format  Units   Label    Explanations

   1- 14  A14    ---     Name     Name of the star
  16- 35  A20    ---     Cat      Catalogue designation (1)
  36- 37  I2     h       RAh      Right ascension 1950 (as obtained from HeB,
                                   the IRAS PSC or SIMBAD)
  39- 40  I2     min     RAm      Right ascension 1950
  42- 46  F5.2   s       RAs      Right ascension 1950
      49  A1     ---     DE-      Declination sign
  50- 51  I2     deg     DEd      Declination 1950 (taken from HeB,
                                   the IRAS PSC or SIMBAD)
  53- 54  I2     arcmin  DEm      Declination 1950
  56- 60  F5.2   arcsec  DEs      []? Declination 1950
      61  A1     ---     u_DEs    [ :*] Uncertainty flag on declination,
                                   * denotes a precision of the order of arcmin
  62- 66  F5.2   mag     PR       []? faintest magnitude of the photometric
                                       range
  69- 73  F5.2   mag     PR2      []? brightest magnitude of the photometric
                                       range
  74- 75  A2     ---     n_PR     [BRIKpg: ] Type of magnitude (2)
  76- 80  F5.2   mag     Vmag     []? Visual magnitude or faintest visual
                                       magnitude (if range of magnitude)(3)
  82- 87  F6.2   mag     Vmag2    []? brightest visual magnitude if range of
                                       magnitude
      88  A1     ---     u_Vmag   [ :?d] 'd' indicates a bracketed value
  89-111  A23    ---     Sp       Spectral characteristics  (4)
 112-156  A45    ---     Other    Other designation (5)
 161-165  A5     ---     IRAS     IRAS source (6)
 167-171  A5     ---     Neb      Nebula (7)
 174-221  A48    ---     Rem      Remarks (8)
 225-284  A60    ---     Refs     Other references (9)

Note (1): see details on the various designations in file "liste2.txt"

Note (2): The largest photometric range known from published data.
     B, V, R and I indicate that the given magnitudes were obtained
     by using filters of the Johnson-Cousins UBVRI system
     pg indicates photographically measured magnitudes
     K indicates that magnitudes are measured through the 2.2 micrometer
     filter of the Johnson JHKLM system.
Note (3): The visual (V) magnitude is given, when the photometric range
    listed in the previous column is not visual. However, instead of a
    single V value, the range in V is given, whenever it is smaller than
    that measured through another passband or determined photographically.
Note (4): The spectral characteristics, such as spectral type,
    luminosity class, emission lines (e) in the optical spectrum and the
    detection of a shell (sh) spectrum, are given. If several spectral
    types are known, they are separated by a slash. Note that the
    determination of the spectral type depends on the studied wavelength
    region, and is influenced by the variability in the spectral lines. We
    also like to mention that a clear distinction between Beq or Bep
    objects has not been made. However, in some cases the historically
    employed classification is given.
Note (5): The other designations are listed in alphabetic order with a
    maximum of three. They are given to avoid confusions with other
    identifications, and for the reader's convenience, in cases when
    different names are frequently used in the literature. The
    abbreviations are explained below. When any confusion exists about the
    possible optical identification of an IRAS source, or when different
    designations refer to the same optical object, they are separated by
    the notation =?, followed by the name of the source.
Note (6): Listed are the confirmed detections of IRAS at or near the
    optically identified source. The source of the data is given behind
    the abbreviation used which are:
        N: No IRAS source
        Y: Iras source.
        ?: IRAS detection hole, see Weintraub 1990
        O: Offset between optical- and IRAS-source
Note (7): When it is known that the star is associated with a nebula,
    it is indicated by the letter Y (Yes), otherwise by the letter N (No).
    For unknown cases, the entries in the column are empty. The references
    from which the listed informations are obtained are given behind these
    letters.
Note (8): Any special remark found in the literature, such as
    near-IR excess, degree of linear polarization, detection of a nearby
    companion or of binarity, and the evolutionary status of an object, is
    given. The remarks and their references are separated by a dash.
    Abbreviations used in the remarks:
         Bin:      Binary
         Cand:     Candidate
         Class Be: Classical Be-star
         Comp:     Companion
         DST:      Double star
         Ecl Bin:  Eclipsing Binary
         Em:       Emission
         HHO:      Herbig-Haro object
         HP(I):    High (Intrinsic) Pol, 1-3%
         L_*:      Stellar luminosity
         LBV:      Luminous Blue Variable
         LP(I):    Low (Intrinsic) Pol, ≤ 1%
         NIRE:     Near Infrared Excess
         N PN:     No Planetary Nebula
         Neb:      Nebula
         Obs Reg:  Obscured Region
         PN:       Planetary Nebula
         Pol:      Polarization
         Poss:     Possible
         Ref Neb:  Reflection Nebula
         Reg:      Region
         Rej:      Rejected see sect. 3.3. and Table 2.
         Sc:       Source
         Sp T:     Spectral Type
         Symb:     Symbiotic star
         Var:      Variable
         VHP(I):   Very High (Intrinsic) Pol, ≥ 3%
    The numbered remarks mean the following:
         (1) Sp. char. XY Per w=Aep+sh
         (2) Refl. Neb-HeB, DST?-FiM
         (3) Neb like star-HeB
         (4) High L_*+PN?+Ring Neb-HeB
         (5) No IRAS sc-BeC
         (6) Triangle Neb-HeB
         (7) Bin?-FiM
         (8) Close to LSS 3027A=CPD-61 3587-SeE
         (9) HAEBE? or B[e]?
        (10) in Obs Reg-HeR
        (11) N PN+HII Reg-ArC
        (12) Neb or Star?-HeB
        (13) No IRAS sc-BeC
        (14) Two faint Comps-HeR
        (15) On edge of small dark cloud-HeB
        (16) No IRAS sc-BeC
        (17) N PN+Symb?-ArC, LBV?-SoB
        (18) Norm. Be?-HeB
    The references are indicated by a 3-letter detailed in
    the "References in the tables" section below.
Note (9): Additional references of the objects mentioned in other
    columns. All the references indicate the published lists where the
    star has been quoted and the ones which are used to collect the given
    information.  The references are indicated by a 3-letter detailed in
    the "References in the tables" section below.


References in the tables:
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  [AlS]= Allen and Swings 1976, A&A, 47, 293 (1976A&A....47..293A)
  [AoS]= Acker. A., Ochsenbein, F., Stenholm, B., Tylenda, B., Marcout, J.,
          Schohn, C. 1992, The Strasbourg-ESO catalogue of Galactic Planetary
          Nebula - Part I&II (see catalog V/84)
  [ArC]= Acker, A., Chopinet, M., Pottasch, S.R., Stenholm, B.
          1987, A&AS, 71, 165 (1987A&AS...71..163A)
  [BaS]= Bhatt, H.C., Sagar, R. 1992, A&AS, 92, 473 (1992A&AS...92..473B)
  [BeC]= Berrilli, F., Corciulo, G., Ingrosso, G., Lorenzetti, D., Nisini, B.,
          Strafella, F. 1992, ApJ, 398, 254 (1992ApJ...398..254B)
  [BiD]= Bidelman, W.P. 1976, in IAU Colloq., Be and Shell Stars,
          ed. A. Slettebak, p457.
  [BiM]= Bidelman, W.P. 1954, ApJS, 1, 175 (1954ApJS....1..175B)
  [BiT]= Bibo, E.A., The, P.S. 1991, A&AS, 89, 319 (1991A&AS...89..319B)
  [BoH]= Bopp, B.W., Howell, B.S. 1989, PASP, 101, 981 (1989PASP..101..981B)
  [BoW]= Bogaert, E., Waelkens, C. 1990, In Int. Colloq., The infrared spectral
          region of stars, eds. C. Jaschek and Y. Andrillat, p345
  [CaH]= Carlson, E.D., Henize, K.G. 1979, Vistas in Astronomy, 23, 213.
          (1979VA.....23..213C)
  [CiD]= Ciatti, F., D'Odorico, S., Mammano, A. 1974, A&A 34, 181.
          (1974A&A....34..181C)
  [CoN]= O'Connell, D.J.K. 1951, MNRAS, 111, 111 (1951MNRAS.111..111O)
  [DeB]= Davies, J.K, Evans, A., Bode, M.F., Whittet, D.C.B.
          1990, MNRAS, 247, 517 (1990MNRAS.247..517D)
  [DoH]= Dong, Y.S., Hu, J.Y. 1991, Chin. A&A, 15, 275 (1991ChA&A..15..275D)
  [FiM]= Finkezeller, U., Mundt, R. 1984, A&AS, 55, 109 (1984A&AS...55..109F)
  [GeH]= McGregor, P.J., Hyland, A.R., Hillier, D.J. 1989, ApJ, 324, 1071
          (1988ApJ...324.1071M)
  [HeB]= Herbig, G.H., Bell, K.R., 1988; Third Catalog of Emission-Line Stars
          of the Orion Population, Lick Obs Bull., No. 1111, University of
          California (see catalog V/73)
  [HeM]= Heydari-Malayeri, M. 1988, A&A, 202, 240 (1988A&A...202..240H)
  [HeR]= Herbig, G.H., Rao, N.K. 1972, ApJ, 174, 401 (1972ApJ...174..401H)
  [HiS]= Hillenbrand, L.A., Strom, S.E., Vrba, F.J., Keene, J.
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          1991, AJ, 101, 1013 (1991AJ....101.1013H)
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  [TiS]= This paper.
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(End)                                           Patricia Bauer [CDS] 06-Dec-1993