Deuteration and evolution in the massive star formation process - The role of surface chemistry

Free Access

Issue		A&A Volume 575, March 2015


Article Number		A87
Number of page(s)		34
Section		Interstellar and circumstellar matter
DOI		https://doi.org/10.1051/0004-6361/201424753
Published online		02 March 2015

Online material

Table 3

Derived line parameters of NH₃(1,1).

Table 4

Same as Table 3 for the NH₃(2,2) transitions.

Table 5

Derived line parameters of ortho-NH₂D(1_1,1−1_0,1) for all sources observed in this line.

Table 6

Integrated area of the ortho- and para-NH₂D lines (Cols. 1 and 2, respectively), and their ratio (Col. 3).

Table 8

Rotation temperatures and total column densities for CH₃OH, ¹³CH₃OH, and CH₂DOH derived from rotation diagrams, unless when specified differently.

© ESO, 2015

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