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UBVRI PHOTOMETRY OF SN 1994D IN NGC-4526
WU, H; YAN, HJ; ZOU, ZL
1995-02-01
Source PublicationASTRONOMY & ASTROPHYSICS
Volume294Issue:1Pages:L9-L12
AbstractIn this paper, we present UBVRI photometric results of SN 1994D which covers the period from March 11 to April 4. All these data were obtained with a Ford 2048x2048 CCD, which has been attached to the 60/90 cm Schmidt telescope in Xinglong station, BAO. The light curves indicate that the supernova is a normal type Ia, a good distance indicator of its parent galaxy. The distance modulus of NGC 4526 is given as 30.07 +/- 0.42.
KeywordSupernovae Sn 1994d Photometry Distance
Indexed BySCI
Language英语
WOS IDWOS:A1995QH14800003
Citation statistics
Cited Times:3[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/8958
Collection光学天文研究部
Affiliation1.CHINESE ACAD SCI, BEIJING ASTRON OBSERV, BEIJING 100080, PEOPLES R CHINA
2.TIANJIN NORMAL UNIV, DEPT PHYS, TIANJIN 300074, PEOPLES R CHINA
Recommended Citation
GB/T 7714
WU, H,YAN, HJ,ZOU, ZL. UBVRI PHOTOMETRY OF SN 1994D IN NGC-4526[J]. ASTRONOMY & ASTROPHYSICS,1995,294(1):L9-L12.
APA WU, H,YAN, HJ,&ZOU, ZL.(1995).UBVRI PHOTOMETRY OF SN 1994D IN NGC-4526.ASTRONOMY & ASTROPHYSICS,294(1),L9-L12.
MLA WU, H,et al."UBVRI PHOTOMETRY OF SN 1994D IN NGC-4526".ASTRONOMY & ASTROPHYSICS 294.1(1995):L9-L12.
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