Gaia Data Release 2 distances and peculiar velocities for Galactic black hole transients
Gaia Data Release 2 distances and peculiar velocities for Galactic black hole transients
We report on a first census of Galactic black hole X-ray binary (BHXRB)
properties with the second data release (DR2) of Gaia, focusing on
dynamically confirmed and strong candidate BH transients. Gaia DR2
provides five-parameter astrometric solutions including position,
parallax and proper motion for 11 out of a sample of 24 systems.
Distance estimates are tested with parallax inversion as well as
Bayesian inference. We derive an empirically motivated characteristic
scalelength of L = 2.17 ± 0.12 kpc for this BHXRB population to
infer distances based upon an exponentially decreasing space density
prior. Geometric DR2 parallaxes provide new, independent distance
estimates, but the faintness of this population in quiescence results in
relatively large fractional distance uncertainties. Despite this, DR2
estimates generally agree with the distances found in the literature.
The most discrepant case is BW Cir, for which detailed studies of the
donor star have suggested a distant location at ≳25 kpc. The large
parallax and relatively high proper motion measured by DR2 instead
indicate significantly smaller distances, suggesting that the source
might be amongst the nearest of XRBs. However, both larger and smaller
distances create problems for the interpretation of the source, and
follow-up data are required to resolve its true nature. DR2 also
provides a first distance estimate to one source, MAXI J1820+070, and
novel proper motion estimates for seven sources. Peculiar velocities
relative to Galactic rotation exceed ≈ 50 km s-1 for the
bulk of the sample, with a median system kinetic energy of peculiar
motion of ˜ 5 × 1047 erg. BW Cir could be a new
high-velocity BHXRB if its astrometry is confirmed. A putative
anticorrelation between peculiar velocity and BH mass is found, as
expected in mass-dependent BH kick formation channels, but this trend
remains weak in the DR2 data.
accretion, accretion discs, parallaxes, proper motions, stars: black holes, stars: distances
2642-2655
Gandhi, Poshak
5bc3b5af-42b0-4dd8-8f1f-f74048d4d4a9
Rao, Anjali
3a3aa402-cf58-4724-9e63-fe9fdc6f39a6
Johnson, Michael A. C.
33a0d8cb-491b-4b3f-b193-540a331ac705
Paice, John A.
0ccafe5a-82d8-40bf-8b73-f71a841ac550
Maccarone, Thomas J.
c2f1d87b-e2ef-4e33-b09f-a2861d917ea8
May 2019
Gandhi, Poshak
5bc3b5af-42b0-4dd8-8f1f-f74048d4d4a9
Rao, Anjali
3a3aa402-cf58-4724-9e63-fe9fdc6f39a6
Johnson, Michael A. C.
33a0d8cb-491b-4b3f-b193-540a331ac705
Paice, John A.
0ccafe5a-82d8-40bf-8b73-f71a841ac550
Maccarone, Thomas J.
c2f1d87b-e2ef-4e33-b09f-a2861d917ea8
Gandhi, Poshak, Rao, Anjali, Johnson, Michael A. C., Paice, John A. and Maccarone, Thomas J.
(2019)
Gaia Data Release 2 distances and peculiar velocities for Galactic black hole transients.
Monthly Notices of the Royal Astronomical Society, 485 (2), .
(doi:10.1093/mnras/stz438).
Abstract
We report on a first census of Galactic black hole X-ray binary (BHXRB)
properties with the second data release (DR2) of Gaia, focusing on
dynamically confirmed and strong candidate BH transients. Gaia DR2
provides five-parameter astrometric solutions including position,
parallax and proper motion for 11 out of a sample of 24 systems.
Distance estimates are tested with parallax inversion as well as
Bayesian inference. We derive an empirically motivated characteristic
scalelength of L = 2.17 ± 0.12 kpc for this BHXRB population to
infer distances based upon an exponentially decreasing space density
prior. Geometric DR2 parallaxes provide new, independent distance
estimates, but the faintness of this population in quiescence results in
relatively large fractional distance uncertainties. Despite this, DR2
estimates generally agree with the distances found in the literature.
The most discrepant case is BW Cir, for which detailed studies of the
donor star have suggested a distant location at ≳25 kpc. The large
parallax and relatively high proper motion measured by DR2 instead
indicate significantly smaller distances, suggesting that the source
might be amongst the nearest of XRBs. However, both larger and smaller
distances create problems for the interpretation of the source, and
follow-up data are required to resolve its true nature. DR2 also
provides a first distance estimate to one source, MAXI J1820+070, and
novel proper motion estimates for seven sources. Peculiar velocities
relative to Galactic rotation exceed ≈ 50 km s-1 for the
bulk of the sample, with a median system kinetic energy of peculiar
motion of ˜ 5 × 1047 erg. BW Cir could be a new
high-velocity BHXRB if its astrometry is confirmed. A putative
anticorrelation between peculiar velocity and BH mass is found, as
expected in mass-dependent BH kick formation channels, but this trend
remains weak in the DR2 data.
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Accepted/In Press date: 4 February 2019
e-pub ahead of print date: 14 March 2019
Published date: May 2019
Keywords:
accretion, accretion discs, parallaxes, proper motions, stars: black holes, stars: distances
Identifiers
Local EPrints ID: 430017
URI: http://eprints.soton.ac.uk/id/eprint/430017
ISSN: 1365-2966
PURE UUID: 2054fb94-354d-4799-a814-8b2b23ddbf6c
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Date deposited: 10 Apr 2019 16:30
Last modified: 16 Mar 2024 04:20
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Contributors
Author:
Anjali Rao
Author:
Michael A. C. Johnson
Author:
John A. Paice
Author:
Thomas J. Maccarone
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