Galactic Center Project Pages

Radio

In the context of this project, comparing radio and X-ray emission is particularly important because emission at both wavelengths can result from non-thermal processes. Many observations have been taken in the radio (see also the transient pages).

• 90 cm (330 MHz): Nord et al.

• 21 cm (neutral H): Lang et al., reduction in progress.

• 20 cm (1.5 GHz): Yusef-Zadeh et al.

• 6 cm polarimetry (5 GHz): Lang et al., reduction in progress.

• 3.6 cm (8.4 GHz) on the inner 10': Bower et al., reduction in progress.

Contacts: Lang, Nord, Kassim, Yusef-Zadeh, Bower

Mid-IR

Infrared

X-ray

Transients