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

F. Fontani; G. Busquet; Aina Palau; P. Caselli; Á. Sánchez-Monge; J. C. Tan; M. Audard

doi:10.1051/0004-6361/201424753

Home

All issues

Volume 575 (March 2015)

A&A, 575 (2015) A87

Online Material

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

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.