Super massive star clusters: from superwinds to a cooling catastrophe and the re-processing of the injected gas
The presence of compact and massive star clusters is a characteristic property of many starburst and interacting galaxies. Their extreme mechanical and...
Super Star Clusters and Supergalactic Winds: The Case of M82
Recent results from Hubble Space Telescope (HST) have resolved starbursts as collections of small young stellar clusters. We have elaborated tep{Melo04} a...
Super star clusters (SSCs) are young massive objects typically observed in starburst galaxies. They consist of millions of stars occupying volumes only several...
We summarize our results based on observations with the NIRI camera on the Gemini North telescope of three Hii galaxies (Mrk 36, UM 408 and UM 461), obtained to...
Here we stress some of the major differences between supergalactic winds and giant superbubbles evolving into the giant low density haloes of galaxies. Both...
Superdense massive galaxies in the nearby universe
At high-z the most superdense massive galaxies are supposed to be the result of gas-rich mergers resulting in compact remnant (Khochfar & Silk (2006); Naab et...
Superdense Massive Galaxies in the Nearby Universe
At high-z the most superdense massive galaxies are supposed to be the result of gas-rich mergers resulting in compact remnant. After this, dry mergers are...