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Molecular Gas and Dust at<i>z</i> = 2.6 in SMM J14011+0252: A Strongly Lensed Ultraluminous Galaxy, Not a Huge Massive Disk
ASTROPHYSICAL JOURNAL, no. 1 (2003): 37-48
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We used the IRAM interferometer to detect CO ( 3 2), CO ( 7 6), and 1.3 mm dust continuum emission from the submillimeter galaxy SMM J14011+0252 at z = 2:6. Contrary to a recent claim that the CO was extended over 6."6 (57 kpc), the new data yield a size of 2" x less than or equal to0."5 for the CO and the dust. Although previous results ...More
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