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J/MNRAS/287/293     BR photometry of EUVE sources (Maoz+ 1997)
================================================================================
Evidence for a new class of extreme ultraviolet sources
       Maoz D., Ofek E.O., Shemi A.
      <Mon. Not. R. Astron. Soc. 287, 293 (1997)>
      =1997MNRAS.287..293M      (SIMBAD/NED BibCode)
================================================================================
ADC_Keywords: X-ray sources; Ultraviolet ; Photometry
Keywords: stars: activity - stars: neutron - novae, cataclysmic variables -
          white dwarfs - X-rays: stars.

Abstract:
    Most of the sources detected in the extreme ultraviolet
    (EUV; 100-600{AA}) by the ROSAT/WFC and EUVE all-sky surveys have been
    identified with active late-type stars and hot white dwarfs that are
    near enough to the Earth to escape absorption by interstellar gas.
    However, about 15 per cent of EUV sources are as yet unidentified with
    any optical counterparts. We examine whether the unidentified EUV
    sources may consist of the same population of late-type stars and
    white dwarfs. We present B and R photometry of stars in the fields of
    seven of the unidentified EUV sources. We detect in the optical the
    entire main-sequence and white dwarf population out to the greatest
    distances where they could still avoid absorption. We use
    colour-magnitude diagrams to demonstrate that, in most of the fields,
    none of the observed stars has the colours and magnitudes of late-type
    dwarfs at distances less than 100pc. Similarly, none of the observed
    stars is a white dwarf within 500pc that is hot enough to be a EUV
    emitter. The unidentified EUV sources we study are not detected in
    X-rays, while cataclysmic variables, X-ray binaries, and active
    galactic nuclei generally are. We conclude that some of the EUV
    sources may be a new class of nearby objects, which are either very
    faint at optical bands or which mimic the colours and magnitudes of
    distant late-type stars or cool white dwarfs. One candidate for
    optically faint objects is isolated old neutron stars, slowly
    accreting interstellar matter. Such neutron stars are expected to be
    abundant in the Galaxy, and have not been unambiguously detected.

File Summary:
--------------------------------------------------------------------------------
  FileName      Lrecl  Records   Explanations
--------------------------------------------------------------------------------
ReadMe             80        .   This file
table1             81        7   Unidentified EUV sources
tab2-8             75      446   BR photometry for unidentified EUV sources
table9             76       23   X-ray visibility of EUV-detected CVs
tables.tex        120      622   LaTeX version of the tables
--------------------------------------------------------------------------------

See also:
     J/ApJS/93/569 : First EUVE source catalogue (Bowyer+, 1994)
            II/203 : Second Extreme Ultra-Violet Explorer Catalog (2EUVE, 1996)
  J/MNRAS/274/1165 : The 2RE Source Catalogue (Pye+ 1995)

Byte-by-byte Description of file: table1
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   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1- 13  A13   ---     EUVE      EUV source name (EUVE or RE)
  16- 29  A14   ---     Band      EUV band
  32- 33  I2    h       RAh       Right ascension (J2000)
  35- 36  I2    min     RAm       Right ascension (J2000)
  38- 39  I2    s       RAs       Right ascension (J2000)
      42  A1    ---     DE-       Declination sign
  43- 44  I2    deg     DEd       Declination (J2000)
  46- 47  I2    arcmin  DEm       Declination (J2000)
  49- 50  I2    arcsec  DEs       Declination (J2000)
  54- 56  I3    deg     GLON      Galactic longitude
  59- 61  I3    deg     GLAT      Galactic latitude
  64- 71  A8 "DD/MM/YY" Date      Observation date
  73- 76  I4    s       Bexp      Time of B exposition
  78- 81  I4    s       Rexp      Time of R exposition
--------------------------------------------------------------------------------

Byte-by-byte Description of file: tab2-8
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   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1- 13  A13   ---     EUVE      EUV source name
  15- 17  I3    ---     Star      Star number in the EUVE field
  19- 23  F5.1  arcsec  Sep       Separation
  25- 30  F6.1  arcsec  oRA       Offset in right ascension (1)
  32- 37  F6.1  arcsec  oDE       Offset in declination (1)
  39- 44  F6.3  mag     Bmag      B magnitude
  46- 50  F5.3  mag   e_Bmag      rms uncertainty on Bmag
  52- 57  F6.3  mag     Rmag      R magnitude
  59- 63  F5.3  mag   e_Rmag      rms uncertainty on Rmag
  65- 69  F5.3  mag     B-R       B-R colour
  71- 75  F5.3  mag   e_B-R       rms uncertainty on B-R
--------------------------------------------------------------------------------
Note (1): Positions (J2000) are relative to:
           RA=07h15m50s, DE=+14{deg}10'18" for EUVE 0715+141
           RA=08h07m59s, DE=+21{deg}04'12" for EUVE 0807+210
           RA=08h47m13s, DE=+59{deg}47'00" for RE 0847+594
           RA=09h22m29s, DE=+71{deg}10'06" for EUVE 9022+711
           RA=16h36m34s, DE=-28{deg}32'00" for EUVE 1636-285
           RA=20h53m35s, DE=-17{deg}33'54" for EUVE 2053-175
           RA=21h14m41s, DE=+50{deg}18'12" for EUVE 2114+503
--------------------------------------------------------------------------------

Byte-by-byte Description of file: table9
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   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1- 13  A13   ---     Name      Star name
  15- 23  A9    ---     Type      Stellar type
  25- 30  F6.1  ct/ks   EUVE100   ? EUVE survey at 100{AA} counts
      31  A1    ---   n_EUVE100   [*] *: EUVE observations with the
                                          Deep Survey Telescope
  32- 34  I3    ct/ks e_EUVE100   ? rms uncertainty on EUVE100
  36- 37  I2    ct/ks   EUVE200   ? EUVE survey at 200{AA} counts
  39- 40  I2    ct/ks e_EUVE200   ? rms uncertainty on EUVE200
  42- 43  I2    ct/ks   EUVE400   ? EUVE survey at 400{AA} counts
  45- 46  I2    ct/ks e_EUVE400   ? rms uncertainty on EUVE400
  48- 49  I2    ct/ks   EUVE600   ? EUVE survey at 600{AA} counts
  51- 52  I2    ct/ks e_EUVE600   ? rms uncertainty on EUVE600
  54- 56  I3    ct/ks   WFC100    ? ROSAT WFC survey at 100{AA} counts
  58- 59  I2    ct/ks e_WFC100    ? rms uncertainty on WFC100
  61- 63  I3    ct/ks   WFC150    ? ROSAT WFC survey at 150{AA} counts
  65- 66  I2    ct/ks e_WFC150    ? rms uncertainty on WFC150
  68- 72  I5    ct/ks   XRT       ? ROSAT XRT survey at 0.1-2.4keV counts
  74- 76  I3    ct/ks e_XRT       ? rms uncertainty on XRT
--------------------------------------------------------------------------------

Acknowledgements: Dan Maoz <dani@wise.tau.ac.il>
================================================================================
(End)                           James Marcout, Patricia Bauer [CDS]  24-Oct-1997

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