Volume 578, June 2015
|Number of page(s)||15|
|Section||Stellar structure and evolution|
|Published online||15 June 2015|
Water maser spectra of the detected sources. Note that some objects were observed more than once. The x-axis is the velocity with respect to the local standard of rest (kinematical definition) in km s-1, and the y-axis is flux density in Jansky. The spectra in the left column show the full scale in flux density, and a range of 200 km s-1 in velocity (except in the case of IRAS 18113−2503, which is shown with a velocity range of 600 km s-1). The spectra in the right column are the same as the corresponding ones in the left column, but with a restricted scale in flux density and/or velocity, to better show weak or narrow spectral features.
|Open with DEXTER|
© ESO, 2015
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