Abstract
Galactic winds are expected to be nearly omnipresent in dwarf galaxies based on theoretical considerations and several indirect observational evidences. The direct observational proof for their presence is far more elusive, contrary to the widespread expectation that dwarf galaxies are very favourable places to observe galactic winds. Interstingly, there is much better direct observational evidence for galactic winds from massive galaxies. I review critically the different methods, their relative sucesses to detect galactic winds in dwarf galaxies, and also comment on the future observational possibilities.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.