Category Astronomy/Space

Star Formation in Distant Galaxy Clusters

Star formation in distant galaxy clusters

The galaxy cluster Abell 1689 as seen by Hubble. The mass in the cluster acts as a gravitational lens, distorting the light from background galaxies into blueish arcs of light. Abell 1689 is relatively close by, but astronomers have now spotted clusters in the early universe via their lensing of even more remote, luminous galaxies, and have studied the star formation underway in their outer regions. Credit: NASA, N. Benitez (JHU), T. Broadhurst (Racah Institute of Physics/The Hebrew University), H. Ford (JHU), M. Clampin (STScI), G. Hartig (STScI), G. Illingworth (UCO/Lick Observatory), the ACS Science Team and ESA

The first stars appeared ~100 million years after the big bang, and ever since then stars and star formation processes have lit up the cosmos, producing heavy elements, planets,...

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Hubble watches the Icy Blue Wings of Hen 2-437

Hubble image of planetary nebula Hen 2-437

In this cosmic snapshot, the spectacularly symmetrical wings of Hen 2-437 show up in a magnificent icy blue hue. Hen 2-437 is a planetary nebula, one of around 3,000 such objects known to reside within the Milky Way. Credit: ESA (European Space Agency)/Hubble & NASA, Acknowledgement: Judy Schmidt

Located in the faint northern constellation of Vulpecula (The Fox), Hen 2-437 was first identified in 1946 by Rudolph Minkowski, who later also discovered the famous and equally beautiful M2-9 (otherwise known as the Twin Jet Nebula). Hen 2-437 was added to a catalog of planetary nebula over 2 decades later by astronomer and NASA astronaut Karl Gordon Henize.

Planetary nebulae such as Hen 2-437 form when an aging low-mass star—such as the sun—reaches the final stages of life...

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Proto-Planet has 2 Masters

An illustration shows the HD 142527 binary star system from data captured by the Atacama Large Millimeter/submillimeter Array. The red body orbiting the center represents the low-mass companion star.

An illustration shows the HD 142527 binary star system from data captured by the Atacama Large Millimeter/submillimeter Array. The red body orbiting the center represents the low-mass companion star. Click image for a larger version. Illustration by B. Saxton/NRAO/AUI/NSF

Rice Uni Assistant Professor Andrea Isella presented images of binary system HD 142527 by Atacama Large Millimeter/submillimeter Array (ALMA) radio telescope at the annual meeting of the American Association for the Advancement of Science in Washington, D.C. The system has long been known to harbor a planet-forming corona of dust and gas, but ALMA images are providing more detail than ever and allowing for better analysis of the system’s contents and mechanics.

Isella studies the formation of planetary systems...

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Caught in the act: Astronomers find a Rare Supernova ‘Impostor’ in a nearby Galaxy

The galaxy NGC 300.

The galaxy NGC 300, home to the unusual system Binder and her colleagues studied. The spiral galaxy is over 6 million light years away.NASA/JPL-Caltech/OCIW

A star pretending to be a supernova mystery illustrates the importance of being in the right place at the right time. Such was the case in May 2010 when an amateur South African astronomer pointed his telescope toward NGC300, a nearby galaxy. He discovered what appeared to be a supernova—a massive star ending its life in a blaze of glory. After a star explodes as a supernova, it usually leaves behind either a black hole or a neutron star—the collapsed, high-density core of the former star. Neither should be visible to Earth after a few weeks. But this supernova—SN 2010da—still was.
“SN 2010da is what we call a ‘supernova impost...

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