PROBABLE OPTICAL COUNTERPART OF THE ECLIPSING MILLISECOND PULSAR SYSTEM, 1957+20

被引：25

作者：

KULKARNI, SR

DJORGOVSKI, S

FRUCHTER, AS

机构：

[1] PRINCETON UNIV,JOSEPH HENRY LABS,PRINCETON,NJ 08544

[2] PRINCETON UNIV,DEPT PHYS,PRINCETON,NJ 08544

来源：

NATURE | 1988年 / 334卷 / 6182期

关键词：

D O I：

10.1038/334504a0

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

引用

页码：504 / 506

页数：3

共 6 条

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NATURE, 1988, 333 (6170) :237-239

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[3] NATURE AND EVOLUTION OF THE ECLIPSING MILLISECOND BINARY PULSAR PSR1957+20 [J].

KLUZNIAK, W ;

RUDERMAN, M ;

SHAHAM, J ;

TAVANI, M .

NATURE, 1988, 334 (6179) :225-227

[4] THE OPTICAL LUMINOSITY OF VERY FAST PULSARS [J].

PACINI, F ;

SALVATI, M .

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[5] ABLATING DWARF MODEL FOR ECLIPSING MILLISECOND PULSAR 1957+20 [J].

PHINNEY, ES ;

EVANS, CR ;

BLANDFORD, RD ;

KULKARNI, SR .

NATURE, 1988, 333 (6176) :832-834

[6] DAOPHOT - A COMPUTER-PROGRAM FOR CROWDED-FIELD STELLAR PHOTOMETRY [J].

STETSON, PB .

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 1987, 99 (613) :191-222

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