OPTICAL POLARIZATION OF THE CRAB-LIKE SUPERNOVA REMNANT 0540-693 IN THE LARGE MAGELLANIC CLOUD

被引：21

作者：

CHANAN, GA ^{[1
]}

HELFAND, DJ ^{[1
]}

机构：

[1] COLUMBIA UNIV,NEW YORK,NY 10027

来源：

ASTROPHYSICAL JOURNAL | 1990年 / 352卷 / 01期

关键词：

Galaxies: Magellanic Clouds; Nebulae: Crab nebula; Nebulae: Individual (0540-693); Nebulae: Supernova remnants; Polarization; Radiation mechanisms;

D O I：

10.1086/168524

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We have measured the linear optical (V band) polarization in the nebula surrounding the Large Magellanic Cloud pulsar 0540-693 and find a positive result (integrated over the nebula) of P = 5.6% ± 1.0%, oriented at an angle 79° ± 5° east of north. Our technique corrects for but does not determine the interstellar polarization, which may be of order 2%. This result is similar to the integrated optical polarization of the Crab Nebula and is strong confirmation of a synchrotron origin for the 0540 nebular emission.

引用

页码：167 / 171

页数：5

共 12 条

[1]

[Anonymous], 1976, ASTROPHYSICAL QUANTI

[2]

[Anonymous], 1956, ASTROPHYS J SUPPL S

[3] AN OPTICAL SYNCHROTRON NEBULA AROUND THE X-RAY PULSAR 0540-693 IN THE LARGE MAGELLANIC CLOUD [J].