galaxies tagged posts

MAS July Monthly Meeting

The Magellanic Stream: A Case Study in Interacting Galaxies

Scott Lucchini

Two of the Milky Way’s nearest neighbors, the Large and Small Magellanic Clouds, have been dancing around each other for billions of years. This dance has led to a huge amount of gas getting thrown from their disks and out into what we know as the Magellanic Stream. In my work, I run high resolution simulations of these interactions to better constrain the history and future of the Magellanic System. Some of our recent results have shown that a warm circumgalactic medium of warm gas around the Magellanic Clouds may play a large role in the formation and current properties of the Stream and that the Stream may be up to five times closer than previously thought...

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May Monthly MAS Meeting

Galactic Structures: Where do they come from? Where do they go?

Our observations of galaxies, from nearby to the edges of the observable universe, reveal striking diversity of size, environment, composition, and apparent structure. Ranging from the clumpy irregulars, through the massive round ellipticals, to the coherent disks — probing the mechanisms responsible for these formations in nature requires a wide range of investigative tools from theoretical observations to detailed spectroscopic observations. Barred spirals comprise 50% of the observed population of nearby disk galaxies yet the physical mechanisms that create and sustain these features are not well understood despite persistent study for nearly 200 years...

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