  Context. Stellar bow shocks have been studied not only observationally, but
also theoretically since the late 1980s. Only a few catalogues of them exist.
The bow shocks show emission along all the electromagnetic spectrum, but they
are detected more easily in infrared wavelengths. The release of new and
high-quality infrared data eases the discovery and subsequent study of new
objects. Aims. We search stellar bow-shock candidates associated with nearby
runaway stars, and gather them together with those found elsewhere, to enlarge
the list of the E-BOSS first release. We aim to characterize the bow-shock
candidates and provide a database suitable for statistical studies. We
investigate the low-frequency radio emission at the position of the bow-shock
features, that can contribute to further studies of high-energy emission from
these objects. Methods. We considered samples from different literature sources
and searched for bow-shaped structures associated with stars in the Wide-field
Infrared Survey Explorer (WISE) images. We looked for each bow-shock candidate
on centimeter radio surveys. Results. We reunited 45 bow-shock candidates and
generated composed WISE images to show the emission in different infrared
bands. Among them there are new sources, previously studied objects, and bow
shocks found serendipitously. Five bow shocks show evidence of radio emission.
Conclusions. Stellar bow shocks constitute an active field with open questions
and enormous amounts of data to be analyzed. Future research at all wavelengths
databases, and use of instruments like Gaia, will provide a more complete
picture of these objects. For instance, infrared spectral energy distributions
can give information about physical parameters of the bow shock matter. In
addition, dedicated high-sensitivity radio observations can help to understand
the radio-$\gamma$ connection.
