METHANOL SOURCE IN ORION AT 1.2 CENTIMETERS

被引：24

作者：

CHUI, MF

CHEUNG, AC

MATSAKIS, D

TOWNES, CH

CARDIASMENOS, AG

机构：

[1] UNIV CALIF, DEPT PHYS, BERKELEY, CA 94720 USA

[2] UNIV MASSACHUSETTS, DEPT ELECT & COMP ENGN, AMHERST, MA 01002 USA

来源：

ASTROPHYSICAL JOURNAL | 1974年 / 187卷 / 01期

关键词：

D O I：

10.1086/181382

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：L19 / L21

页数：3

共 7 条

[1] DETECTION OF METHYL ALCOHOL IN ORION AT A WAVELENGTH OF - 1 CENTIMETER [J].

BARRETT, AH ;

SCHWARTZ, PR ;

WATERS, JW .

ASTROPHYSICAL JOURNAL, 1971, 168 (03) :L101-&

[2] STUDIES OF INTERSTELLAR FORMAMIDE [J].

GOTTLIEB, CA ;

PALMER, P ;

RICKARD, LJ ;

ZUCKERMAN, B .

ASTROPHYSICAL JOURNAL, 1973, 182 (03) :699-710

[3]

HARVEY PH, IN PRESS

[4] NEW INTERSTELLAR METHANOL LINES [J].

KUTNER, ML ;

THADDEUS, P ;

PENZIAS, AA ;

WILSON, RW ;

JEFFERTS, KB .

ASTROPHYSICAL JOURNAL, 1973, 183 (01) :L27-L30

[5]

LISZT HS, IN PRESS

[6] DETECTION OF 41-30 (E2) LINE OF INTERSTELLAR METHYL ALCOHOL [J].

TURNER, BE ;

WRIXON, GT ;

GORDON, MA .

ASTROPHYSICAL JOURNAL, 1972, 177 (03) :609-&

[7]

YNGVESSON KS, IN PRESS

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