This tag is associated with 36 posts

Minor Mergers are Minor Players

Once thought to be the main mechanism by which galaxies feed their star formation; the authors of this paper find that minor mergers cannot account for the observed star formation rates of galaxies.

Accretion in Young Stars

What might be causing the accretion rates in newly formed stars to remain so high?

A Faint Black Hole?

The authors report the discovery of perhaps the faintest black hole x-ray binary. But this conclusion is limited by the uncertainty in the distance to the object.

Blank Sky But Not Blank Information

Archival data are able to place constraints on the origin of supernova 2011fe.

What Fed Sgr A* its Latest Meal?

The black hole at the center of our galaxy, Sgr A*, is a very picky eater. However, with the discovery of the G2 cloud, astronomers have had the opportunity to watch the infrequent feeding process in Sgr A* in action. While the origin of this cloud is still debated, research is beginning to suggest that G2 is a gas cloud that was ripped away from a giant star in orbit around our galaxy’s central black hole.

Galaxy in a Bottle: Simulating Spiral Galaxy Formation

How do simulations of galaxy formation stack up against each other and against observations? Find out with the Aquila project, a comparo of many different codes in current use.

The Changing Faces of Active Galactic Nuclei

Has a multi-wavelength study of AGN across a large redshift range revealed that these energetic giants do not impact upon their host galaxy as significantly as previously thought?

Progenitors of AM CVn systems

The progenitors of a special type of cataclysmic variable, AM CVn, and possibly supernovae have been found.

Chandra Observes Sgr A* Rejecting Material

Sgr A* – the supermassive black hole sitting in the center of the Milky Way – is often referred to as a ‘starved’ black hole, meaning that it swallows very little of the nearby cosmic gas and dust. The authors of this paper observed Sgr A* with the Chandra X-ray telescope for 3 mega seconds, throughout which only 1% of the gas available to Sgr A* actually accreted onto the black hole. It swallows cold gas, while rejecting hot gas – ejecting the matter back into space.

Another hungry black hole devours a star

Maksym et al. investigate a possible tidal flare event in Abell 1795.

Follow us on Twitter

Like us on Facebook

Astroplots Astroplots to explore astronomy research through data representation.


Our sister site

Enter your email address to subscribe to Astrobites and receive notifications of new posts by email.