========================================================================== J/A+A/475/915 L1489IRS observed by the submillimeter array (Brinch+, 2007) The following files can be converted to FITS (extension .fit .fgz or .fiZ) list.dat ========================================================================== Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/475/915 ==========================================================================
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Beginning of ReadMe : J/A+A/475/915 L1489IRS observed by the submillimeter array (Brinch+, 2007) ================================================================================ A deeply embedded young protoplanetary disk around L1489 IRS observed by the submillimeter array. Brinch, C., Crapsi, A., Jorgensen, J., K., Hogerheijde, M., R., Hill, T. <Astron. Astrophys. 475, 915 (2007)> =2007A&A...475..915B ================================================================================ ADC_Keywords: YSOs ; Infrared sources ; Millimetric/submm sources ; Radio lines Keywords: stars: formation - circumstellar matter - ISM: individual objects: L1489 IRS - submillimeter Description: Submillimeter Array observations of the Young Stellar Object L1489IRS (IRAS 04016+2610). These include images of the continuum at 267 GHz (1.12 mm) and line emission of the HCO+ J=3-2 transition at 267.55762 GHz. The HCO+ image is available in two different (u,v)-weighting schemes, natural and uniform, optimizing for S/N and resolution respectively. The continuum image is only available in uniform weighting. The synthesized beam size is 1". Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 04 04 47.5 +26 19 42 LDN 1489 = MLB 3-6 04 04 43.0 +26 18 57 LDN 1489 IRS = IRAS 04016+2610 ----------------------------------------------------------
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