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 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 278 108 Herbig Ae/Be members and candidate members table2.dat 237 23 F-type PMS stars, potential candidates and those with unknown spectral type table3.dat 252 23 Extreme emission line objects (EELOs) table4a.dat 227 32 Other early type emission line stars with IR-excess from AIS table4b.dat 224 87 Other early type emission line stars with IR-excess from DoH table5.dat 232 14 Non-emission line early type shell stars and young stellar candidates table6.dat 237 35 Emission line stars rejected as Herbig Ae/Be candidates -------------------------------------------------------------------------------- Byte-per-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: [AlE]= Allen, D.A. 1984, Proc. Astr. Soc. Aus., 5,39 (1984PASAu...5..369A 1984PASAu...5..369A) [AlS]= Allen and Swings 1976, A&A, 47, 293 (1976A&A....47..293A 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 1987A&AS...71..163A) [BaS]= Bhatt, H.C., Sagar, R. 1992, A&AS, 92, 473 (1992A&AS...92..473B 1992A&AS...92..473B) [BeC]= Berrilli, F., Corciulo, G., Ingrosso, G., Lorenzetti, D., Nisini, B., Strafella, F. 1992, ApJ, 398, 254 (1992ApJ...398..254B 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 1954ApJS....1..175B) [BiT]= Bibo, E.A., The, P.S. 1991, A&AS, 89, 319 (1991A&AS...89..319B 1991A&AS...89..319B) [BoH]= Bopp, B.W., Howell, B.S. 1989, PASP, 101, 981 (1989PASP..101..981B 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 1979VA.....23..213C) [CiD]= Ciatti, F., D'Odorico, S., Mammano, A. 1974, A&A 34, 181. (1974A&A....34..181C 1974A&A....34..181C) [CoN]= O'Connell, D.J.K. 1951, MNRAS, 111, 111 (1951MNRAS.111..111O 1951MNRAS.111..111O) [DeB]= Davies, J.K, Evans, A., Bode, M.F., Whittet, D.C.B. 1990, MNRAS, 247, 517 (1990MNRAS.247..517D 1990MNRAS.247..517D) [DoH]= Dong, Y.S., Hu, J.Y. 1991, Chin. A&A, 15, 275 (1991ChA&A..15..275D 1991ChA&A..15..275D) [FiM]= Finkezeller, U., Mundt, R. 1984, A&AS, 55, 109 (1984A&AS...55..109F 1984A&AS...55..109F) [GeH]= McGregor, P.J., Hyland, A.R., Hillier, D.J. 1989, ApJ, 324, 1071 (1988ApJ...324.1071M 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 1988A&A...202..240H) [HeR]= Herbig, G.H., Rao, N.K. 1972, ApJ, 174, 401 (1972ApJ...174..401H 1972ApJ...174..401H) [HiS]= Hillenbrand, L.A., Strom, S.E., Vrba, F.J., Keene, J. 1992, ApJ, 397, 613 (1992ApJ...397..613H 1992ApJ...397..613H) [HuH]= Hughes, J.D., Hartigan, P., Graham, J.A., Emerson, J.P., Marang, F. 1991, AJ, 101, 1013 (1991AJ....101.1013H 1991AJ....101.1013H) [IDS]= Jeffers, H.M., v.d. Bos, W.H., Greeby, F.M. 1963, Catalogue of visual double stars, Publ. Lick Obs, 21, 17+263+804. [ImA]= Imhoff, C., Appenzeller, I. 1987, in Scientific Accomplishments of the IUE, ed. Y. Kondo, 295. [JaJ]= Jaschek, M., Andrillat, Y., Jaschek, C. 1991, A&A, 250, 127. (1991A&A...250..127J 1991A&A...250..127J) [JaS]= Jaschek, M., Jaschek, C., Egret, D. 1986, A&A, 158, 325. (1986A&A...158..325J 1986A&A...158..325J) [OuE]= Oudmaijer, R.D., v.d. Veen, W.E.C.J., Waters, L.B.F.M., Trams, N.R., Waelkens, C., Engelsman, E., 1992; A&AS 96, 625 (1992A&AS...96..625O 1992A&AS...96..625O) [PaP]= Parthasarathy, M., Pottasch, S.R. 1989; A&A 225, 521. (1989A&A...225..521P 1989A&A...225..521P) [SeE]= Steenman, H., The, P.S. 1989, Ap&SS, 161, 75 (1989Ap&SS.161...75S 1989Ap&SS.161...75S) [SeT]= Slettebak, A. 1986, PASP, 98, 867 (1986PASP...98..867S 1986PASP...98..867S) [SoB]= Shore, S.N., Brown, D.N., Bopp, B.W., Robinson, C.R., Sandulaek, N., Feldman, P.D. 1990, ApJS, 73, 461 (1990ApJS...73..461S 1990ApJS...73..461S) [SoN]= Strom, K.M., Newton, G., Strom, S.E., Seaman, R.L., Carrasco, L. Cruz-Gonzales, I., Serrano, A. 1989, ApJS, 71, 183. (1989ApJS...71..183S 1989ApJS...71..183S) [TiS]= This paper. [WaS]= Walter, F.M., Skinner, S.L., Boyd, W.T. 1990, PASP, 102, 754. (1990PASP..102..754W 1990PASP..102..754W) [WeJ]= Weaver, W.B., Jones, G. 1992, ApJS, 78, 239 (1992ApJS...78..239W 1992ApJS...78..239W) [WeT]= Weintraub, D.A. 1990, ApJS, 74, 575 (1990ApJS...74..575W 1990ApJS...74..575W) [WiH]= de Winter, D., Hu, J.Y., The, P.S., in preparation. [WiT]= de Winter, D., The, P.S. 1991, Ap&SS, 166, 99 (1990Ap&SS.166...99D 1990Ap&SS.166...99D) [ZiS]= Zickgraf, F.-J., Schulte-Ladbeck, R.E. 1989, A&A, 214, 274. (1989A&A...214..274Z 1989A&A...214..274Z)
(End) Patricia Bauer [CDS] 06-Dec-1993
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line