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When a star's core contracts to a critical point, a series of nuclear reactions is unleashed. This fusion staves off core collapse for a time—but only until the core is composed largely of iron, which can no longer sustain star fusion.

In a microsecond, the core may reach temperatures of billions of degrees Celsius. Iron atoms become crushed so closely together that the repulsive forces of their nuclei create a recoil of the squeezed core—a bounce that causes the star to explode as a supernova and give birth to an enormous, superheated, shock wave.

Supernovae also occur in binary star systems. Smaller stars, up to eight times the mass of our own sun, typically evolve into white dwarves.

A star condensed to this size, about that of Earth, is very dense and thus has strong enough gravitational pull to gather material from the system's second star if it is close enough.

If a white dwarf takes on enough mass it reaches a level called the Chandrasekhar Limit. At this point the pressure at its center will become so great that runaway fusion occurs and the star detonates in a thermonuclear supernova.

A supernova can light the sky up for weeks, and the massive transfer of matter and energy leaves behind a very different star. Typically only a tiny core of neutrons, a spinning neutron star , is left to evidence a supernova.

Neutron stars give off radio waves in a steady stream or, as pulsars, in intermittent bursts. If a star was so massive at least ten times the size of our sun that it leaves behind a large core, a new phenomenon will occur.

Because such a burned-out core has no energy source to fuse, and thus produces no outward pressure, it may become engulfed by its own gravity and turn into a cosmic sinkhole for energy and matter—a black hole.

Supernovae Learn more about what happens when stars explode. We have successfully implemented over projects in Austria, Croatia, Slovenia and Slovakia.

Sustainability is at the center of what we do. Supernova connects the best locations with the ideal tenants. Advanced design and top quality construction form the foundation of successful management throughout the lifecycle of the real estate.

Our buy-and-hold investment strategy is the basis of our active end asset management through which we aim to continuously improve the quality of our properties and ensure they meet and maintain our Supernova standards.

Investing in real estate means adding value. We remain focused on continuing to increase the size of our portfolio. Our many years of experience help us to recognize potential that might not be apparent to others.

We understand that a successful transaction is a win-win for everyone involved. For all our acquisitions we apply strict investment criteria: physical property visits by two general managers, legal, tax and technical due diligences procedures as well as valuations by independent appraisers.

Active asset management is an ongoing process. The main focus of our active asset management approach is to enhance the quality and value of our real estate as well as increase the appeal of our objects for both customers and tenants.

This includes the reduction of overall operating costs, optimizing the tenant mix and creating new rental space. Further advancement of real estate is a process, and it requires input from many experts in a variety of fields: architects, civil engineers, leasing specialists and financing professionals.

Supernova unites all of these skill sets under one roof. Everyday contact with public officials, our renters and our clients means that we can quickly react to new opportunities and new challenges.

Our dynamic portfolio is continuously being optimized by our highly skilled portfolio managers. We invest our money into selected projects, and we regularly market existing real estate.

Our main aim is sustainability and therefore we always try to achieve extended timeframes in holding a real estate by passing all compliance tests with excellence.

Due to our exceptionally high level of management skills, we are often assigned with the center and asset management, even after a successful sale has taken place.

Supernova builds the best locations and finds the best tenants for them. Decades of successful cooperation with international brands are complemented by our tenant pool that is made up of high-quality local renters.

Our focus is on long-term, successful partnerships. Through our local center management, we ensure access to a competent point of contact at any time.

Our large number of projects means that we can offer our tenants a presence in the best locations throughout the region. The Supernova Zadar Shopping Center has two floors, and since its opening in as the largest shopping center in this popular vacation destination, it has become equally well liked by tourists and locals.

It is only one of the 48 stores that Supernova took over from the bauMax Portfolio in the fall of The Welserheimb Palace, constructed in , was acquired in In coordination with the commission responsible for historic preservationas well as the office which handles monuments, the property underwent comprehensive reconstruction and refurbishment in and This shopping center, located in the middle of the Rudnik business district, was opened in More than 60 shops and approximately 27, square meters of retail space made it the largest shopping center in this area of the city.

We are investing in the future of real estate.

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Cappellaro, M. Doggett, D. URL consultato il 24 marzo Howell, 'et al. L37—L40, DOI : Fryer, K. URL consultato il 24 marzo archiviato dall' url originale il 27 marzo Mazzali et al.

Lieb, H. Yau, A rigorous examination of the Chandrasekhar theory of stellar collapse , in Astrophysical Journal , vol. Canal, J. Isern, M.

Hernanz, E. Khokhlov, E. Mueller, P. Hoeflich, Light curves of Type IA supernova models with different explosion mechanisms , in Astronomy and Astrophysics , vol.

Röpke, W. L1—L4, DOI : Hillebrandt, J. Macri et al. URL consultato il 25 marzo Colgate, Supernovae as a standard candle for cosmology , in Astrophysical Journal , vol.

Richmond, Late stages of evolution for low-mass stars , Rochester Institute of Technology. URL consultato il 27 marzo Postnov, L.

URL consultato il 27 marzo archiviato dall' url originale il 26 settembre Howell et al. Tanaka et al. Woosley, H. URL consultato il 7 giugno URL consultato il 7 giugno archiviato dall' url originale il 12 marzo Heger et al.

URL consultato il 26 marzo Nomoto, M. Tanaka, N. Tominaga, K. Maeda, Hypernovae, gamma-ray bursts, and first stars , in New Astronomy Reviews , vol.

URL consultato il 5 maggio Blandford, C. McKee, Fluid dynamics of relativistic blast waves , in Physics of Fluids , vol.

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Woosley, A. URL consultato l'8 giugno URL consultato l'8 aprile Kunugise, K. Hayden et al. URL consultato il 9 aprile Smartt, Progenitors of core-collapse supernovae , in Annual Review of Astronomy and Astrophysics , vol.

Naeye, R. Barbon, F. Ciatti, L. URL consultato il 31 marzo Li et al. The observed luminosity functions and fractions of supernovae in a complete sample , in Monthly Notices of the Royal Astronomical Society , vol.

URL consultato il 2 aprile Richardson et al. Frail et al. L—L, DOI : Hoflich, P. Kumar, J. Wheeler, Neutron star kicks and supernova asymmetry , in Cosmic explosions in three dimensions: Asymmetries in supernovae and gamma-ray bursts , Cambridge University Press , L—L, Bibcode : ApJ URL consultato il 6 aprile archiviato dall' url originale il 31 dicembre URL consultato il 6 aprile URL consultato il 10 aprile Woosley, W.

Heavy elements are only produced in supernovae, so all of us carry the remnants of these distant explosions within our own bodies. Supernovae add enriching elements to space clouds of dust and gas, further interstellar diversity, and produce a shock wave that compresses clouds of gas to aid new star formation.

But only a select few stars become supernovae. Many stars cool in later life to end their days as white dwarfs and, later, black dwarfs.

But massive stars, many times larger than our own sun, may create a supernova when their core's fusion process runs out of fuel.

Star fusion provides a constant outward pressure, which exists in balance with the star's own mass-driven, inward gravitational pull.

When fusion slows, outbound pressure drops and the star's core begins to condense under gravity—becoming ever denser and hotter. To outward appearances, such stars begin growing, swelling into bodies known as red supergiants.

But at their cores, shrinking continues, making a supernova imminent. When a star's core contracts to a critical point, a series of nuclear reactions is unleashed.

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