SIMULTANEOUS OBSERVATION OF DIRECT AND RAMAN-SCATTERED O-VI LINES IN THE SYMBIOTIC NOVA RR-TELESCOPII

被引:33
作者
ESPEY, BR
SCHULTELADBECK, RE
KRISS, GA
HAMANN, F
SCHMID, HM
JOHNSON, JJ
机构
[1] UNIV PITTSBURGH,DEPT PHYS & ASTRON,PITTSBURGH,PA 15260
[2] UNIV CALIF SAN DIEGO,CTR ASTROPHYS & SPACE SCI,LA JOLLA,CA 92093
[3] AUSTRALIAN NATL UNIV,MT STROMLO & SIDING SPRING OBSERV,CANBERRA,ACT 2611,AUSTRALIA
[4] UNIV WISCONSIN,DEPT ASTRON,MADISON,WI 53706
基金
美国国家科学基金会; 美国国家航空航天局;
关键词
ATOMIC PROCESSES; BINARIES; SYMBIOTIC; STARS; INDIVIDUAL (RR TELESCOPII); ULTRAVIOLET;
D O I
10.1086/309764
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The optical spectra of some symbiotic binaries show two lines in the red region of the spectrum that cannot be identified with any known allowed or forbidden transitions. A case has been made that these lines are Raman-scattered O VI lambda lambda 1032, 1038 emission lines. We present simultaneous far-UV and optical spectra of the symbiotic nova RR Tel, obtained with the Hopkins Ultraviolet Telescope and the Angle-Australian Telescope during the Astro-2 Space Shuttle mission. These data show the first coincident detection of the strong O VI lambda lambda 1032, 1038 doublet and lambda lambda 6825, 7082 emission lines. The latter display strong linear polarization and provide new information on the structure of the nebular material. Our observations provide strong evidence for the Raman effect in RR Tel.
引用
收藏
页码:L61 / L64
页数:4
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