2023ApJ...958L..16V


Query : 2023ApJ...958L..16V

2023ApJ...958L..16V - Astrophys. J., 958, L16 (2023/November-3)

Discovery of X-Ray Polarization from the Black Hole Transient Swift J1727.8-1613.

VELEDINA A., MULERI F., DOVCIAK M., POUTANEN J., RATHEESH A., CAPITANIO F., MATT G., SOFFITTA P., TENNANT A.F., NEGRO M., KAARET P., COSTA E., INGRAM A., SVOBODA J., KRAWCZYNSKI H., BIANCHI S., STEINER J.F., GARCIA J.A., KRAVTSOV V., NITINDALA A.P., EWING M., MASTROSERIO G., MARINUCCI A., URSINI F., TOMBESI F., TSYGANKOV S.S., YANG Y.-J., WEISSKOPF M.C., TRUSHKIN S.A., EGRON E., IACOLINA M.N., PILIA M., MARRA L., MIKUSINCOVA R., NATHAN E., PARRA M., PETRUCCI P.-O., PODGORNY J., TUGLIANI S., ZANE S., ZHANG W., AGUDO I., ANTONELLI L.A., BACHETTI M., BALDINI L., BAUMGARTNER W.H., BELLAZZINI R., BONGIORNO S.D., BONINO R., BREZ A., BUCCIANTINI N., CASTELLANO S., CAVAZZUTI E., CHEN C.-T., CIPRINI S., DE ROSA A., DEL MONTE E., DI GESU L., DI LALLA N., DI MARCO A., DONNARUMMA I., DOROSHENKO V., EHLERT S.R., ENOTO T., EVANGELISTA Y., FABIANI S., FERRAZZOLI R., GUNJI S., HAYASHIDA K., HEYL J., IWAKIRI W., JORSTAD S.G., KARAS V., KISLAT F., KITAGUCHI T., KOLODZIEJCZAK J.J., LA MONACA F., LATRONICO L., LIODAKIS I., MALDERA S., MANFREDA A., MARIN F., MARSCHER A.P., MARSHALL H.L., MASSARO F., MITSUISHI I., MIZUNO T., NG C.-Y., O'DELL S.L., OMODEI N., OPPEDISANO C., PAPITTO A., PAVLOV G.G., PEIRSON A.L., PERRI M., PESCE-ROLLINS M., POSSENTI A., PUCCETTI S., RAMSEY B.D., RANKIN J., ROBERTS O.J., ROMANI R.W., SGRO C., SLANE P., SPANDRE G., SWARTZ D.A., TAMAGAWA T., TAVECCHIO F., TAVERNA R., TAWARA Y., THOMAS N.E., TROIS A., TUROLLA R., VINK J., WU K. and XIE F.

Abstract (from CDS):

We report the first detection of the X-ray polarization of the bright transient Swift J1727.8-1613 with the Imaging X-ray Polarimetry Explorer. The observation was performed at the beginning of the 2023 discovery outburst, when the source resided in the bright hard state. We find a time- and energy-averaged polarization degree of 4.1% ± 0.2% and a polarization angle of 2.°2 ± 1.°3 (errors at 68% confidence level; this translates to ∼20σ significance of the polarization detection). This finding suggests that the hot corona emitting the bulk of the detected X-rays is elongated, rather than spherical. The X-ray polarization angle is consistent with that found in submillimeter wavelengths. Since the submillimeter polarization was found to be aligned with the jet direction in other X-ray binaries, this indicates that the corona is elongated orthogonal to the jet.

Abstract Copyright: © 2023. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Accretion - X-ray astronomy - Low-mass x-ray binary stars - Polarimetry - Astrophysical black holes

Simbad objects: 15

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Number of rows : 15
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 1A 0620-00 HXB 06 22 44.5423857312 -00 20 44.290460544           K3V-K7V 1144 0
2 MCG-05-23-016 Sy2 09 47 40.1332188528 -30 56 55.960779696   14.10 13.69 12.44   ~ 611 0
3 NGC 4151 Sy1 12 10 32.5759813872 +39 24 21.063527532   12.18 11.48     ~ 3938 2
4 NAME Circinus Galaxy Sy2 14 13 09.906 -65 20 20.47   10.89 9.84 10.6 10.0 ~ 1331 1
5 V* IL Lup HXB 15 47 08.2768672752 -47 40 10.284587760         15.624 ~ 532 1
6 V* V381 Nor HXB 15 50 58.6637920704 -56 28 35.258385000           K3III 1254 0
7 V* V821 Ara LXB 17 02 49.3876391280 -48 47 23.087954544         15.322 ~ 2237 0
8 SWIFT J1727.8-1613 HXB 17 27 43.3135483931 -16 12 19.062182343           ~ 140 0
9 V* V4641 Sgr HXB 18 19 21.6343259256 -25 24 25.849595952     13.654 13.479 13.139 B9III 530 0
10 MAXI J1820+070 LXB 18 20 21.9423816480 +07 11 07.284859440           ~ 511 0
11 [KRL2007b] 353 HXB 19 08 53.080 +09 23 04.84     15.80     ~ 125 0
12 Granat 1915+105 HXB 19 15 11.55576 +10 56 44.9052           ~ 2810 0
13 HD 226868 HXB 19 58 21.6757355952 +35 12 05.784512688 9.38 9.72 8.91 8.42   O9.7Iabpvar 4590 0
14 V* V404 Cyg HXB 20 24 03.8247037434 +33 52 01.961154861           G9/K0III/V 1370 0
15 V* V1521 Cyg HXB 20 32 25.78 +40 57 27.9           WN4/5-6/7 2035 2

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