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2018ApJ...854..125T - Astrophys. J., 854, 125-125 (2018/February-3)
A radio frequency study of the accreting millisecond X-ray pulsar, IGR J16597-3704 in the globular cluster NGC 6256.
TETARENKO A.J., BAHRAMIAN A., WIJNANDS R., HEINKE C.O., MACCARONE T.J., MILLER-JONES J.C.A., STRADER J., CHOMIUK L., DEGENAAR N., SIVAKOFF G.R., ALTAMIRANO D., DELLER A.T., KENNEA J.A., LI K.L., PLOTKIN R.M., RUSSELL T.D. and SHAW A.W.
Abstract (from CDS):
Abstract Copyright: © 2018. The American Astronomical Society. All rights reserved.
Journal keyword(s): globular clusters: individual: NGC 6256 - ISM: jets and outflows - radio continuum: stars - stars: individual: IGR J16597-3704 - stars: neutron - X-rays: binaries
Simbad objects: 28
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