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2018ApJ...856..158K - Astrophys. J., 856, 158-158 (2018/April-1)
Toward understanding the B[e] phenomenon. VII. AS 386, a single-lined binary with a candidate black hole component.
KHOKHLOV S.A., MIROSHNICHENKO A.S., ZHARIKOV S.V., MANSET N., ARKHAROV A.A., EFIMOVA N., KLIMANOV S., LARIONOV V.M., KUSAKIN A.V., KOKUMBAEVA R.I., OMAROV C.T., KURATOV K.S., KURATOVA A.K., RUDY R.J., LAAG E.A., CRAWFORD K.B., SWIFT T.K., PUETTER R.C., PERRY R.B., CHOJNOWSKI S.D., AGISHEV A., CATON D.B., HAWKINS R.L., SMITH A.B., REICHART D.E., KOUPRIANOV V.V. and HAISLIP J.B.
Abstract (from CDS):
Abstract Copyright: © 2018. The American Astronomical Society. All rights reserved.
Journal keyword(s): binaries: spectroscopic - stars: emission-line, Be - stars: individual: AS 386
VizieR on-line data: <Available at CDS (J/ApJ/856/158): table1.dat table2.dat table3.dat table4.dat>
CDS comments: Star #18 is probably 2MASS J20103939+3818577 (not in SIMBAD).
Simbad objects: 9
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