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## (from tabmap V6.0 (2016-08-18)) 2024-05-18T06:27:48
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#-- J/A+A/347/47 High galactic latitude RASS X-ray sources. II. (Beuermann+, 1999)
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#---Table: J/A+A/347/47/./notes.dat Individual notes of table3.dat (51 records)
# Name A15 --- RASS name
# Note A63 --- Text of the note
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Name |Note
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013242.8-655434|AM Herculis binary (Burwitz et al., 1996A&A...310L..25B)
015400.9-594749|AM Herculis binary (Beuermann & Thomas, 1993, Adv. Space Res.
015400.9-594749|13 (12), 115). The variable X-ray source is not contained in
015400.9-594749|the RASS BSC. The J2000 X-ray position derived from the PET
015400.9-594749|is 1 54 00.8 -59 48 10.
030313.9-474214|CCD image shows galaxy with bright nucleus within 3" from X-ray
030313.9-474214|position, B = 18.2 (ROE finding chart). The 14mag star 20" NE
030313.9-474214|of spectral type ~K1 is probably unrelated to the X-ray source
045929.4-222953|Our R filter image shows a galaxy with a bright core. Our two
045929.4-222953|spectra show red-shifted absorption lines of the galaxy but no
045929.4-222953|emission lines.
050146.2-035927|AM Herculis binary (Burwitz et al., 1998, in preparation)
051214.5-324140|Soft Intermediate Polar (Burwitz et al., 1997A&A...327..183B)
051541.7+010528|AM Herculis binary (Shafter et al., 1995ApJ...443..319S)
054747.2-195609|The CCD image shows galaxy with bright nucleus 5" W of X-ray
054747.2-195609|position. Our spectrum misses the nucleus and shows a weak
054747.2-195609|absorption spectrum with z=0.055:. A probably unrelated late
054747.2-195609|F star is 31" E
060033.1-270918|AM Herculis binary (Beuermann & Burwitz, 1995, ASP Conf. Ser.
060033.1-270918| 85, 99)
080621.7-152715|Intermediate Polar. The highly variable X-ray source is not
080621.7-152715|contained in the RASS BSC. The J2000 X-ray position derived
080621.7-152715|from the PET is 8 06 22.2 15 27 14
083650.3-155328|White dwarf. Only a non-calibrated spectrum is available. The
083650.3-155328|X-ray source is not contained in the RASS BSC. The J2000 X-ray
083650.3-155328|position derived from the PET is. 8 36 52.2 15 53 51
085909.5+053703|AM Herculis binary (Beuermann & Burwitz 1995, ASP Conf. Ser.
085909.5+053703|85, 99), V = 16.5-18.7
095308.6+145841|AM Herculis binary (Beuermann & Burwitz, 1995, ASP Conf. Ser.
095308.6+145841|85, 99)
101718.0+291439|This active galaxy is known as CASG59 (Salzer et al., 1995,
101718.0+291439|Cat. <J/AJ/109/2376>)
104614.2+525600|The Hamburg survey lists this source as an AGN. Our segments of
104614.2+525600|blue and red spectra miss MgII and H{beta}. H{gamma} is very
104614.2+525600|weak. Weaker spectral features yield z=0.510+/-0.003.
110842.1+595010|Our spectrum contains only one Balmer line adjacent to a broad
110842.1+595010|Fe-line complex. Interpreting the line as H{beta} yields the
110842.1+595010|quoted redshift.
181810.0+534343|The 90% confidence error circle contains three objects. The
181810.0+534343|V~15 object 15" SW is a G-star, no spectrum is available of the
181810.0+534343|V=14.5 candidate 5" NE and the V ~19 candidate 12" SSE.
202237.8-395412|AM Herculis binary (Burwitz et al., 1996A&A...310L..25B)
203626.2-535222|HR1=~-1 suggests a WD. Candidate 1 is ~20" NW, has B=12, and
203626.2-535222|is of spectral type ~K0; candidate 2 is 10" E, has B=17 and
203626.2-535222|B-V=0.6; candidate 3 is 23" E, has B=16 and B-V=0.9. If the WD
203626.2-535222|is associated with the K-star it should be fainter than B=~15.5
224642.0-520638|Galaxy, no emission lines. Final CR-HR1 values place the source
224642.0-520638|outside our sample.
234939.7-563723|A close pair of a B=13 star of spectral type ~K0 and an ~15mag
234939.7-563723|object is 19" NW, two faint red objects 18" S. The X-ray source
234939.7-563723|is variable and could be an AGN or a CV.
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