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J/A+A/674/A64
  FIFI-LS spectroscopy of Gy 3-7 in outer Galaxy (Le+, 2023)
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2023A&A...674A..64L
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cube/fits
img(gal)
    J/A+A/674/A64/list(c)List of datacubes (10 rows)
    J/A+A/674/A64/table2CO rotational temperature, the number of emitting molecules, and total line luminosities of CO and [OI] lines toward dense cores in Gy 3-7 and IM YSOs from Matuszak et al. (2015A&A...578A..20M) (8 rows)
    J/A+A/674/A64/table4Physical parameters for a subset of YSO candidates with at least 5 photometric data points (12 rows)
    J/A+A/674/A64/tablea1Parameters of the 22 GHz H2O maser lines detected toward CMa l224 with RT4 (7 rows)
    J/A+A/674/A64/tableb1Flux SOFIA FIFI-LS toward the two dense cores within a beam size of 20" (9 rows)
    J/A+A/674/A64/tablec1(c)*Multi-wavelength photometry of YSO candidates in the IRAS field. (Note) (15 rows)
    J/A+A/674/A64/tabled1CO rotational temperature and number of emitting molecules for HM YSOs, derived by fitting the rotational diagram of CO using all and only four available CO transitions (10 rows)
    J/A+A/674/A64/tabled2Far-IR line cooling luminosity of the sample in the Milky Way (MW), LMC, and SMC used to compare with results of this study (29 rows)

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       (c)  indicates tables which contain celestial coordinates 
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