- ... RX J1856.5-3754
- Based on observations collected at the European
Southern Observatory, Paranal, Chile (ESO Programmes 63.H-0416
and 65.H-0643).
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- ... stars
- Given that most radio
pulsars are also isolated, a better name might be "thermally emitting''
neutron stars.
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- ...
East
- In the meantime, the proper motion has been
measured accurately using HST (Walter 2001).
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- ...
images
- Photometry of star X using these images was presented
by Neuhäuser (2001). He finds
,
consistent with (though
substantially less accurate than) our result.
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- ... expected
- We used
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as inferred by Predehl & Schmitt (1995) for distant,
highly absorbed objects. In these, the line of sight samples all
phases of the interstellar medium; hence, the relation may not be
valid locally.
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- ... respectively
- If they are giants, with
(Cox 2000), they would be at
and might be associated with the Sagittarius dwarf galaxy
(Ibata et al. 1995), which is at
and
away from RX J1856.5-3754. Indeed, stars L and C have radial velocities of
,
consistent with being associated.
Star F, with a radial velocity of
,
almost certainly is not associated.
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- ... processes
- Assuming that the disk is optically
thick and radiates as a black body. It is questionable whether these
assumptions are justified for the very low accretion rate considered
here, but given the speculative nature of the presence of an accretion
disk, we felt a more detailed analysis was not warranted.
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