Data reported in Figure 1 correspond to newly detected C2O and lines towards: L1544 (panels A, B, C, D, E and F); L1498 (panels G and H); and Elias 18 (panels I and J). Each panel reports the molecule and its transition. The detection reported in panel G (performed with the Noto-32m telescope) was acquired with a lower resolution than that used for the observations reported in the other panels (IRAM-30m telescope). For clarity we give a larger VLSR scale that allows a better evaluation of the baseline. Table 1 and Table 2 in the paper report information on the spectroscopic parameters and telescope used. Further details are given in Section 2 in the paper. Files are given in FITS and ASCII format for each panel. (3 data files).
URSO, R.G., PALUMBO, M.E., Ceccarelli, C., Balucani, N., Bottinelli, S., CODELLA, C., et al. (2019). VizieR Online Data Catalog: C2O and C3O in low-mass star-forming region [10.26093/cds/vizier.36280072].
VizieR Online Data Catalog: C2O and C3O in low-mass star-forming region
TESTI, Leonardo
2019
Abstract
Data reported in Figure 1 correspond to newly detected C2O and lines towards: L1544 (panels A, B, C, D, E and F); L1498 (panels G and H); and Elias 18 (panels I and J). Each panel reports the molecule and its transition. The detection reported in panel G (performed with the Noto-32m telescope) was acquired with a lower resolution than that used for the observations reported in the other panels (IRAM-30m telescope). For clarity we give a larger VLSR scale that allows a better evaluation of the baseline. Table 1 and Table 2 in the paper report information on the spectroscopic parameters and telescope used. Further details are given in Section 2 in the paper. Files are given in FITS and ASCII format for each panel. (3 data files).I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
