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MAGHMXBCAT - Magellanic Clouds High-Mass X-Ray Binaries Catalog |
HEASARC Archive |
Information on the numbers used to code references is available at CDS. Individual notes on each HMXB are also available for SMC systems and for LMC systems at the same site.
This Browse table contains the combination of 92 HMXBs in the SMC and 36 HMXBs in the LMC which were listed in Tables 1 and 2, respectively, of the published version of this catalog. The HEASARC has added a parameter called cloud_id which can be used to identify which Magellanic Cloud any specified HMXB belongs to (the SMC or the LMC).
High-mass X-ray binaries in the Magellanic Clouds. Liu Q.Z., van Paradijs J., van den Heuvel E.P.J. <Astron. Astrophys. 442, 1135 (2005)> =2005A&A...442.1135L
Name
The source name, generally containing a positional string with rough
information on the its sky location of the HMXB, according to the standard
naming convention hhmm.m+/-ddmm, or variations of lower or higher accuracy.
(Here hh and mm.m indicate the hours and minutes of right ascension, and dd.mm
the declination in degrees and arcminutes). The prefix J indicates a name
based on J2000 coordinates, otherwise 1950 coordinates were used in the name,
and there is no explicit prefix. A small number of the HMXBs have other
types of names, e.g., 'XTE SMC46'.
Xray_Type
The X-ray type of the high-mass X-ray binary:
P: X-ray pulsar (47 in the SMC and 7 in the LMC) T: Transient X-ray source U: Ultra-soft X-ray spectrum. These sources include black-hole candidates; some 'extreme ultra-soft' (EUS) source may be white dwarfs (WDs) on whose surfaces steady nuclear burning takes place.
RA
The Right Ascension of the high-mass X-ray binary. In the original
published version of the catalog table this was given in J2000 equatorial
coordinates and with a precision varying between 0.01 seconds of
time to 1 minute of time. Notice that there is one source in the SMC (XTE
SMC144s) for which no position was specified in this catalog.
Dec
The Declination of the high-mass X-ray binary. In the original
published version of the catalog table this was given in J2000 equatorial
coordinates and with a precision varying between 0.1 arcseconds
to 1 arcminute.
LII
The Galactic Longitude of the high-mass X-ray binary.
BII
The Galactic Latitude of the high-mass X-ray binary.
Optical_Name1
The name or type of the optical counterpart to the HMXB,
if known. An asterisk followed by a number or letter refers to star numbers
used in the finding chart; "star" refers a star in the finding chart that
has not been assigned a number or letter. Many optical counterparts have been
indicated with an H-alpha emission-line object in the SMC by Meyssonier and
Azzopardi (1993, CDS Cat. <J/A+AS/102/451> hereafter MA93) and an SMC member
star by Azzopardi and Vigneau (1982A&AS...50..291A, hereafter AzV), or a
number in a well-known catalog (e.g., GSC, 2MASS, OGLE, MACHO etc.).
Optical_Name2
A second name or type of the optical counterpart to the HMXB,
if known. An asterisk followed by a number or letter refers to star numbers
used in the finding chart; "star" refers a star in the finding chart that
has not been assigned a number or letter. Many optical counterparts have been
indicated with an H-alpha emission-line object in the SMC by Meyssonier and
Azzopardi (1993, CDS Cat. <J/A+AS/102/451> hereafter MA93) and an SMC member
star by Azzopardi and Vigneau (1982A&AS...50..291A, hereafter AzV), or a
number in a well-known catalog (e.g., GSC, 2MASS, OGLE, MACHO etc.).
Ref_Chart
Reference codes for the finding chart(s) for the optical
counterpart. The reference code key can be found at
https://cdsarc.cds.unistra.fr/ftp/cats/J/A+A/442/1135/refs.dat.
Vmag_Flag
This parameter is set to '~' if the associated V magnitude
is considered uncertain.
Vmag
The apparent visual (V) magnitude of the optical counterpart. If
a range of visual magnitudes is known for a source, this parameter lists
the maximum (brightest) magnitude while the parameter vmag_min lists
the minimum (faintest) magnitude.
Vmag_Min
If a range of visual magnitudes is known for a source, this
parameter lists the minimum (faintest) magnitude, while the parameter
vmag lists the maximum (brightest) magnitude.
Bmag
The apparent blue (B) magnitude of the optical counterpart.
Rmag
The apparent red (R) magnitude of the optical counterpart.
BV_Color
The (B-V) color index of the optical counterpart.
UB_Color
The (U-B) color index of the optical counterpart.
Spect_Type
The spectral type of the optical counterpart to the HMXB.
Reddening
The interstellar reddening E(B-V) of the optical counterpart.
If a range of E(B-V) values is known for a source, this parameter lists
the minimum value while the parameter reddening_max lists the maximum value.
Reddening_Max
If a range of E(B-V) values is known for a source, this
parameter lists the maximum value while the parameter reddening lists the
minimum value.
Ref_Photometry
The reference codes for the optical counterpart photometric
information. The reference code key can be found at
https://cdsarc.cds.unistra.fr/ftp/cats/J/A+A/442/1135/refs.dat.
Fx_Limit
If the value of the X-ray flux (fx) is an upper limit rather
than a detection, this flag is set to '<', while, if the value is
considered uncertain, this flag is set to '~'.
Fx
The average observed X-ray flux (density) in microJanskies (µJy) in
the 2 - 10 keV energy range, unless (i) a range of X-ray flux (densities) is
known, in which case this parameter contains the minimum observed X-ray flux
(density) and the parameter fx_max contains the maximum observed X-ray flux
(density), or (ii) the observed X-ray flux (density) is known for
a different energy range, as specified by the (non-blank) value of the
fx_range parameter.
Notice that 1 uJy = 10-29 erg/s/cm2/Hz = 2.4 10-12 erg/s/cm2/keV.
Fx_Max
If a range of X-ray flux (densities) is known for a source, this
parameter contains the maximum observed X-ray flux (density) and the parameter
fx contains the minimum observed X-ray flux (density).
Fx_Range
This parameter contains the energy range corresponding to
the quoted X-ray flux values (fx and fx_max). If blank, the energy range
should be assumed to be 2 - 10 keV.
Ref_Fx
A reference code(s) for the X-ray flux (density) values.
The reference code key can be found at
https://cdsarc.cds.unistra.fr/ftp/cats/J/A+A/442/1135/refs.dat.
Porb
The orbital period of the HMXB, in days.
Porb_Flag
A flag that is set to '?' if the orbital period value is
uncertain.
Pulse_Period
This parameter is the pulse period, in seconds, for those
HMXBs which are X-ray pulsars.
Ref_Period
Reference codes for the source(s) for the orbital and/or
pulsational period information. The reference code key can be found at
https://cdsarc.cds.unistra.fr/ftp/cats/J/A+A/442/1135/refs.dat.
Alt_Name
An alternative name for the HMXB, generally another X-ray
designation.
Cloud_ID
A HEASARC-created parameter that is set to 'SMC' for HMXBs in
the Small Magellanic Cloud and to 'LMC' for those in the Large Magellanic
Cloud.
Class
The HEASARC Browse classification, based on a combination of the
X-ray type and optical spectral type information.