LARGE MAGELLANIC CLOUD SOURCES AT 3.4-CM WAVELENGTH

被引：37

作者：

MCGEE, RX

NEWTON, LM

BUTLER, PW

机构：

[1] Division of Radiophysics, CSIRO, PO Box 76, Epping,NSW,2121, Australia

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1978年 / 183卷 / 03期

关键词：

Galaxies; -; NASA;

D O I：

10.1093/mnras/183.4.799

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Selected regions of the Large Magellanic Cloud have been surveyed at wavelength 3.4 cm with a 2.5 arcmin half-power beamwidth. Improved spectral indices are given for 35 sources in the LMC area. Contour maps of the 30 Doradus nebula and the four important sources to the south of it are presented. © 1978 Royal Astronomical Society. Provided by the NASA Astrophysics Data System.

引用

页码：799 / 804

页数：6

共 12 条

[1]

Bolton J. G., 1975, Australian Journal of Physics, P33

[2] RADIO CONTINUUM OF LARGE MAGELLANIC CLOUD .2. CONTINUUM OBSERVATIONS AT 11 CM WAVELENGTH [J].

BROTEN, NW .

AUSTRALIAN JOURNAL OF PHYSICS, 1972, 25 (05) :599-612

[3]

Clarke J. N., 1976, Australian Journal of Physics, Astrophysical Supplement, P1

[4]

Davies R.D., 1976, MNRAS, V81, P89

[5]

ELLIOTT KH, 1977, ASTRON ASTROPHYS, V55, P187

[6] ISOPHOTOMETRY OF 30 DORADUS NEBULA [J].

FAULKNER, DJ .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1967, 135 (04) :401-&

[7]

Henize K. G., 1956, AP J S, V2, P315

[8]

KERR AR, 1971, RPL185 CSIRO DIV RAD

[9] SUPERNOVA REMNANTS IN LARGE MAGELLANIC CLOUD [J].

MATHEWSON, DS ;

CLARKE, JN .

ASTROPHYSICAL JOURNAL, 1973, 180 (03) :725-738

[10] RECOMBINATION LINES NEAR 6 CM WAVELENGTH IN LARGE MAGELLANIC CLOUD [J].

MCGEE, RX ;

NEWTON, LM ;

BROOKS, JW .

AUSTRALIAN JOURNAL OF PHYSICS, 1974, 27 (05) :729-735

← 1 2 →