II/171              Parenago Catalog of Stars in Orion Nebula   (Parenago 1954)

Machine-Readable version of the Parenago Catalogue of stars in the area of the Orion Nebula Parenago P.P. <Trudy Gos. Astron. Inst. im. Shternberga, 25 (1954)> =1954TrSht..25....1P 1954TrSht..25....1P Malkov O.Yu. <Bull. Inf. CDS 40, 13 (1992)> =1992BICDS..40...13M 1992BICDS..40...13M
ADC_Keywords: Magnitudes, photographic ; Nebulae ; Stars, variable Description: The present catalogue is a machine-readable version of the catalogue of stars in the area of the Orion nebula, published by P.P. Parenago (1954). The sky area between 5h 24m and 5h 36m in right ascension (1900.0) and between -4 and -7 degrees in declination (1900.0), containing the Orion nebula, has been investigated in that work. Ten of variable stars in original Parenago (1954) catalogue had CSV numbers (Kukarkin et al., 1951) but since that time all of them were confirmed as variables and included in GCVS (Kholopov et al., 1985a&b, 1987). We superseded CSV-numbers by GCVS-names in the machine-readable version for the following stars: ------------------------------------------------ Number in CSV-number GCVS-name the catalogue ------------------------------------------------ 1605 606 V372 ORI 1613 607 V373 ORI 1635 608 V374 ORI 1713 609 V375 ORI 1748 610 V387 ORI 1762 100569 V376 ORI 1974 617 V377 ORI 2183 625 V388 ORI 2393 630 V380 ORI 2478 634 V381 ORI ------------------------------------------------ File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file catalog.dat 51 2983 The Parenago Catalogue -------------------------------------------------------------------------------- See also: V/73 : Emission-Line Stars of the Orion Population (Herbig+ 1988) III/177 : H-alpha emission stars in the Orion region (Wiramihardja+ 1993) Byte-by-byte Description of file: catalog.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 A1 --- Member *[*] asterisk if star is a member. 2- 5 I4 --- Parenago Sequential number. 6 A1 --- m_Parenago *[A] Blank for one star 8 I1 h RAh [5] Right Ascension 1900 (hours) 10- 11 I2 min RAm Right Ascension 1900 (minutes) 13- 14 I2 s RAs Right Ascension 1900 (seconds) 15 A1 --- DE- [-] Declination 1900 (sign) 16- 17 I2 deg DEd [4/7] Declination 1900 (degrees) 19- 22 F4.1 arcmin DEm Declination 1900 (minutes) 24- 27 F4.1 mag mpg *[2/18]? Photographic magnitudes. 28 A1 --- n_mpg *[ENS] Flag on mpg 30 A1 --- l_mpv [<] '<' should be read as "mpv fainter than" 31- 34 F4.1 mag mpv [2/18]? photovisual magnitudes, if existing 36- 43 A8 --- GCVS Name of variable star in GCVS II/139 45- 51 A7 --- SpType *Spectral type -------------------------------------------------------------------------------- Note on Member: the asterisk is set if a star is a member of the Orion nebula, blank otherwise. Probably, not every member of the nebula is marked by '*', but as Parenago (1954) noted "it was better to omit some of them (members), than to include nonmember stars" (p.250). Altogether 634 stars have asterisks. Note on m_Parenago: There are two different stars with number 2617 in the catalogue: 2617 and 2617A. Note on mpg: Blank when the star is variable; in that case the corresponding designation from GCVS (Kholopov et al., 1985a&b, 1987) appears in columns 36-45. Note on n_mpg: the flag has the following meaning: 'E' - if photographic magnitude represents approximate estimation of visual or infrared magnitudes; 'N' - if the star is in the nebula and its influence can be perceptible; 'S' - if the influence of the nebula is strong; blank otherwise. Note on SpType: the spectral type (if existing) is a mean value both from literature and from Parenago's classification. The peculiarities 'e', 'ea' (read "e alpha") and 'eb' (read "e beta") mean hydrogen emission at the moment of observations. -------------------------------------------------------------------------------- References: Kholopov P.N., Samus' N.N., Frolov M.S., Goranskij V.P., Gorynya N.A., Kireeva N.N., Kukarkina N.P., Kurochkin N.E, Medvedeva G.I., Perova N.B., Shugarov S.Yu. 1985a, General Catalogue of Variable Stars, Fourth Edition, vol.I, Nauka, Moscow. (Catalog II/139) Kholopov P.N., Samus' N.N., Frolov M.S., Goranskij V.P., Gorynya N.A., Kazarovets E.V., Kireeva N.N., Kukarkina N.P., Kurochkin N.E, Medvedeva G.I., Perova N.B., Rastorguev A.S., Shugarov S.Yu. 1985b, General Catalogue of Variable Stars, Fourth Edition, vol.II, Nauka, Moscow. (Catalog II/139) Kholopov P.N., Samus' N.N., Frolov M.S., Goranskij V.P., Gorynya N.A., Karitskaya E.A., Kazarovets E.V., Kireeva N.N., Kukarkina N.P., Medvedeva G.I., Pastukhova E.N., Perova N.B., Shugarov S.Yu. 1987, General Catalogue of Variable Stars, Fourth Edition, vol.III, Nauka, Moscow. (Catalog II/139) Kukarkin B.V., Parenago P.P., Efremov Yu.I., Kholopov P.N. 1951, Catalogue of Suspected Variable Stars, Moscow. Parenago P.P. 1954, "Trudy Gosudarstvennogo Astronomicheskogo Instituta im Shternberga", vol.25. Historical Notes: The catalogue was keypunched at the CDS and was checked at the Soviet Center of Astronomical Data. It was documented by O.Yu. Malkov in 1992. * 04-Oct-1997: documentation standardized at CDS (F. Ochsenbein)
(End) Malkov O.Yu (25-Feb-1992), Francois Ochsenbein [CDS] 04-Oct-1997
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