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A Catalogue of X-Ray Sources in the Sky Region Between Δ = −73 And

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A Catalogue of X-Ray Sources in the Sky Region Between Δ = −73 And Publ. Astron. Soc. Aust., 1999, 16, 175–205. A Catalogue of X-ray Sources in the Sky Region between = 73 and = +27 M. T. Meliani Instituto Nacional de Pesquisas Espaciais, INPE, Divis˜ao de Astrofsica, CP 515, S. Jose dos Campos-SP, 12201–970 Brazil [email protected] Received 1998 November 23, accepted 1999 April 20 Abstract: This Catalogue lists coordinates, X-ray uxes in dierent energy ranges, magnitudes and colour indices, optical counterparts, orbital periods of binaries, pulsar periods and other characteristics of 226 X-ray sources (HMXBs, LMXBs, pulsars and galaxies) between = 73 and = +27. Keywords: catalogues — X-ray sources: stars, galaxies — stars: binaries, pulsars 1 Introduction 2 The Catalogue The Catalogue lists 226 selected X-ray emitting The Catalogue contents are explained below. The objects with declinations between 73 references cited are listed in numerical and alpha- +27. The information was obtained principally betical order at the end. The Catalogue is available from the technical literature published from 1992 to electronically from the electronic version of Publi- May 1998. Some recently discovered sources, such cations of the Astronomical Society of Australia at as RXTE 1550–56 and RXTE 2123–058, have also http://www.atnf.csiro.au/pasa/16 2/meliani/. been included. The layout of the Catalogue follows First column: The source name related with the standard format used in Bradt & McClintock its sky location in epoch 1950 (B) and/or 2000 (1985) and van Paradijs (1995). However, the (J). The conventional format is hhmmddd, where coordinates for both B1950 and J2000 have been hh and mm indicate the hour and minute of right included, as have the X-ray uxes in six dierent ascension and ddd indicates the declination. If energy ranges. This work updates and complements there is an alternative name, it is also given. the two catalogues referred to in the declination The sources that emit above 30 keV are distin- rang considered. guished. In the Catalogue the sources are ordered according Second column: The rst line gives the type to class (A: LMXBs; B: HMXBs and C: other sources) of source: and right ascension. The numbers in square brackets LMXB: low-mass X-ray binary refer to the publications from which the data were HMXB: high-mass X-ray binary obtained, and additional information is given as key Binary: binaries sources without classication words. The Catalogue classies 60 high-mass X-ray Pulsar binaries (HMXBs), 35 of which have a pulsar; 124 QSO: quasar low-mass X-ray binaries (LMXBs), 8 of which have AGN: active galactic nuclei. a pulsar; 9 binaries, 7 of which have a pulsar; 9 The second line gives: simple pulsars; 7 galaxies; and 1 quasar. There (a) if the source is in a binary system; are 16 other sources without classication. Optical A: atoll source counterparts are known for 82 sources and they are B: X-ray burst source also listed. A list of objects in lexigraphical order D: ‘dipping’ LMXBs is also given in Table 1. G: globular cluster X-ray source The Catalogue will be used to select X-ray sources P: X-ray pulsar to be observed with the MASCO telescope (Villela T: transient X-ray source et al. 1995) that is being constructed to operate in U: ultra-soft X-ray spectrum the range 40 to 5000 keV. The MASCO telescope Z: Z-type. will be launched by balloon at latitude 23 in (b) if the source is a pulsar; Brazil. About one third of the sources emit above SNR: associated with a supernova remnant. 30 keV and are concentrated in the Galactic Centre, The third line gives the type of observation and the main target of the MASCO telescope. source position error: q Astronomical Society of Australia 1999 1323-3580/99/020175$10.00 Downloaded from https://www.cambridge.org/core. IP address: 170.106.33.22, on 26 Sep 2021 at 11:12:00, subject to the Cambridge Core terms of use, available at https://www.cambridge.org/core/terms. https://doi.org/10.1071/AS99175 176 M. T. Meliani Table 1. List of objects in lexigraphical order 3C273 B1226+023 NGC 6712 B1850–087 AV 111 B005017247 NGC 7582 B2315426 BR Cir B1516569 NP 0531 B0531+219 BW Cir B1354645 QV Nor B1538522 UW CrB B1603+260 S84 B0726260 BP CruWra 977 B1223624 SK 160 B0115737 2 CruHD 112091 B1255567 MM Ser B1837+049 GR Mus B1254690 NP Ser B1813140 HD 63666SAO 235515 B0739529 SK-Ph B0532664 HD 65663SAO 250018 B0749600 Ter 2 B1734307 HD 77581GP Vel B0900403 Ter 5 B1745248 HD 110432SAO 252002 B1249637 Ter 6 B1747313 HD 141926SAO 243098 B1555552 KY TrA B1524617 HD 153919V884 Sco B1700377 KZ TrA B1627673 HD 154791 B1704+240 LU TrA B1556605 HD 161103 J174472713 V1333 Aql B1908+005 He3640 B1118615 V1343 AqlSS 433 B1909+048 Hen715V801Cen B1145619 V1405 Aql B1916053 HV 2554 J05286954 V1408 Aql B1957+115 HV 5682 B05139695 V801 Ara B1636536 Kes 73 J1841045 V821 Ara B1659487 Lil 1 B1730335 V395 Car B0921630 LS 992 J081243114 V779 Cen B1119603 LS 1698 B1036565 V822 Cen B1455314 LS 5039 J182621450 V830 Cen B114516141 M15AC211 B1227+119 V850 Cen B1258613 M28 B182124 V691 CrA B1822371 MCG-52316 B0945397 V616 Mon B0620003 MMVel B100945 V2107 Oph B1705250 MSH 1532G320412 B150958 V2116Oph B1729247 N67 B005687164 V2134 Oph B1658298 NCL 101 B1811171 V2216 Oph B1728169 NGC 1068 B0240001 V2293 Oph B1716249 NGC 1851 B0512401 V1055 Ori B0614+091 NGC 4507 B1232396 V4134 Sgr B1755338 NGC 4945 B1304497 V818 Sco B1617155 NGC 5128 B1322427 V926 Sco B1735444 NGC 6440 B1745203 V725 Tau B0535+262 NGC 6441 (star U1) B1746370 UY Vol B0748676 NGC 6624 B1820303 QZ Vul B2000+251 NGC 6652 B1832330 Wack 2134TH3542 B10245732 o: optical Eighth column: Gives the X-ray uxes F x in x: X-ray units of 105 photons cm2 s1 keV1 in the ranges: i: infrared rst line: 2–10 keV (or 01–24 keV for those r: radio. sources indicated by an asterisk). Third column: The rst and second lines give second line: 40–80 keV (or 10–40 keV for those right ascension (RA) and declination (DEC) in epoch sources indicated by an asterisk). 1950. The third line gives the galactic longitude third line: 80–180 keV. and latitude. Ninth column: Gives the X-ray uxes F x in Fourth column: The rst and second lines give units of 105 photons cm2 s1 keV1 in the ranges: the right ascension (RA) and declination (DEC) in rst line: 200–600 keV epoch 2000. second line: 600–1000 keV Fifth column: The optical counterpart, if known, third line: above 1000 keV. and associations. The notation nnEm stands for nn 10m. Sixth column: The magnitude and colour indices Tenth column: of the optical counterpart; rst line: orbital period in days (d) or hours rst line: V (h) second line: B–V second line: pulsar period in seconds (s) or third line: U–B. milliseconds (ms) Seventh column: third line: the X-ray catalogues and experi- rst line: spectral type of optical counterpart ments in which the source was listed and/or second line: interstellar reddening, E BV. detected: Downloaded from https://www.cambridge.org/core. IP address: 170.106.33.22, on 26 Sep 2021 at 11:12:00, subject to the Cambridge Core terms of use, available at https://www.cambridge.org/core/terms. https://doi.org/10.1071/AS99175 Catalogue of X-ray Sources 177 A: Ariel V sky survey (McHardy et al. 1981; Acknowledgments Warwick et al. 1981) This work was supported by the Fundac˜ao de Amparo H: HEAO A-4 sky survey (Levine et al. 1984) a Pesquisa do Estado de S˜ao Paulo (FAPESP) M: MIT OSO-7 sky survey (Markert et al. process numbers 95/09831–2 and 98/07641–0. The 1979) author acknowledges Dr Walter F. Velloso Jr for U: Uhuru sky survey (Forman et al. 1978) his suggestions. X: Catalogue of X-ray binaries (van Paradijs 1995). References As: ASCA Bradt, H. V., & McClintock, J. E. 1983, ARA&A, 21, 13 B: Beppo Sax Forman, W., Jones, C., Cominsky, L., Julien, P., Murray, S., Bb: Broad Band X-ray Telescope (BBXRT) Peters, G., Tanabaum, H., & Giacconi, R. 1978, ApJS, 38, 357 (IV Catalog Uhuru) C: Compton -ray Observatory (Batse, GRO) Levine, A. M., Lang, F. L., Lewin, W. H. G., et al. 1984, Cb: Cos B ApJS, 54, 581 (HEAO1-A4 Catalog) E: Einstein McHardy, I. M., Lawrence, A., Pye, J. P., & Pounds, K. Eg: Egret A. 1981, MNRAS, 197, 893 Exo: Exosat Markert, T. H., Winkler, P. F., Laird, F. N., Clark, G. W., Hearn, D. R., Sprot, G. F., Li, F. K., Bradt, H. V., FII: Figaro II (X- and -ray) Lewin, W. H. G., & Schnopper, H. W. 1979, ApJS, 39, G: Ginga 573 Gr: Granat van Paradijs, J. 1995, in X-ray Binaries, ed. W. H. J. Lewin, Ha: Hakucho J. van Paradijs & E. P. J. van den Heuvel, p. 536 K: Kvant Villela, T., Braga, J., D’ Amico, F., & Jayanthi, U. B. 1995, Adv. Space Res., 15, 98 OAO: Orbiting Astronomical Observatory Warwick, R. S., Marshal, N., Fraser, G. W., Watson, M. G., P: Prognoz 9 Lawrence, A., Page, C. G., Pounds, K. A., & Ricketts, R: ROSAT M. J. 1981, MNRAS, 197, 865 Rx: Rossi X-ray Timing Explorer (RXTE) Zeng, Q., Lou, G. F., & Li, S. Z. 1987, Ap&SS, 132, 263. S: SAS 3 S2: SAS2 SL: Space Lab T: Tenma V: Vela-5 and Vela-6 satellites The symbol (:) that follows some values indicates imprecise data. Downloaded from https://www.cambridge.org/core. IP address: 170.106.33.22, on 26 Sep 2021 at 11:12:00, subject to the Cambridge Core terms of use, available at https://www.cambridge.org/core/terms.
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