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The MAVERIC survey: a hidden pulsar and a black hole candidate in ATCA radio imaging of the globular cluster NGC 6397.

Authors :
Zhao, Yue
Heinke, Craig O
Tudor, Vlad
Bahramian, Arash
Miller-Jones, James C A
Sivakoff, Gregory R
Strader, Jay
Chomiuk, Laura
Shishkovsky, Laura
Maccarone, Thomas J
Pichardo Marcano, Manuel
Gelfand, Joseph D
Source :
Monthly Notices of the Royal Astronomical Society; 04/21/2020, Vol. 493 Issue 4, p6033-6049, 17p
Publication Year :
2020

Abstract

Using a 16.2-h radio observation by the Australia Telescope Compact Array and archival Chandra data, we found >5σ radio counterparts to four known and three new X-ray sources within the half-light radius (r <subscript>h</subscript>) of the Galactic globular cluster NGC 6397. The previously suggested millisecond pulsar (MSP) candidate, U18, is a steep-spectrum (S <subscript>ν</subscript> ∝ ν<superscript>α</superscript>; |$\alpha =-2.0^{+0.4}_{-0.5}$|⁠) radio source with a 5.5-GHz flux density of 54.7 ± 4.3  |$\mu \mathrm{ Jy}$|⁠. We argue that U18 is most likely a 'hidden' MSP that is continuously hidden by plasma shocked at the collision between the winds from the pulsar and companion star. The non-detection of radio pulsations so far is probably the result of enhanced scattering in this shocked wind. On the other hand, we observed the 5.5-GHz flux of the known MSP PSR J1740−5340 (U12) to decrease by a factor of >2.8 during epochs of 1.4-GHz eclipse, indicating that the radio flux is absorbed in its shocked wind. If U18 is indeed a pulsar whose pulsations are scattered, we note the contrast with U12's flux decreases in eclipse, which argues for two different eclipse mechanisms at the same radio frequency. In addition to U12 and U18, we also found radio associations for five other Chandra X-ray sources, four of which are likely background galaxies. The last, U97, which shows strong H α variability, is mysterious; it may be either a quiescent black hole low-mass X-ray binary or something more unusual. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
00358711
Volume :
493
Issue :
4
Database :
Complementary Index
Journal :
Monthly Notices of the Royal Astronomical Society
Publication Type :
Academic Journal
Accession number :
142931607
Full Text :
https://doi.org/10.1093/mnras/staa631