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The Laser Interferometer Space Antenna (LISA) is a proposed space probe to detect and accurately measure gravitational waves—tiny ripples in the fabric of spacetime—from astronomical sources. LISA would be the first dedicated space-based gravitational-wave observatory. It aims to measure gravitational waves directly by using laser interferometry. The LISA concept has a constellation of three spacecraft arranged in an equilateral triangle with sides 2.5 million kilometres long, flying along an Earth-like heliocentric orbit. The distance between the satellites is precisely monitored to detect a passing gravitational wave.
Tryptase is the most abundant secretory granule-derived serine proteinase contained in mast cells and has been used as a marker for mast cell activation. Club cells contain tryptase, which is believed to be responsible for cleaving the hemagglutinin surface protein of influenza A virus, thereby activating it and causing the symptoms of flu.
HM Cancri (also known as HM Cnc or RX J0806.3+1527) is an X-ray binary star system about 1,600 light-years (490 pc; 1.5×1016 km) away. It comprises two dense white dwarfs orbiting each other once every 5.4 minutes, at an estimated distance of only 80,000 kilometres (50,000 mi) apart (about 1/5 the distance between the Earth and the Moon). The two stars orbit each other at speeds in excess of 400 kilometres per second (890,000 mph). The stars are estimated to be about half as massive as the Sun. Like typical white dwarfs, they are extremely dense, being composed of degenerate matter, and so have radii on the order of the Earth's radius. Astronomers believe that the two stars will eventually merge, based on data from many X-ray satellites, such as Chandra X-Ray Observatory, XMM-Newton and the Swift Gamma-Ray Burst Mission. These data show that the orbital period of the two stars is steadily decreasing at a rate of 1.2 milliseconds per year as they thus are getting closer by approximately 60 centimetres (2.0 ft) per day. At this rate, they can be expected to merge in approximately 340,000 years. With a revolution period of 5.4 minutes, HM Cancri is the shortest orbital period binary white dwarf system currently known.
Adam Willaerts was a Dutch Golden Age painter.
An AM Canum Venaticorum star, is a rare type of cataclysmic variable star named after their type star, AM Canum Venaticorum. In these hot blue binary variables, a white dwarf accretes hydrogen-poor matter from a compact companion star.
AM Canum Venaticorum is a hydrogen-deficient cataclysmic variable binary star in the constellation of Canes Venatici. It is the type star of its class of variables, the AM Canum Venaticorum stars. The system consists of a white dwarf gaining matter via an accretion disk from a semi-degenerate or white dwarf companion.
HD 140913 is a star very much like our own Sun located in the northern constellation of Corona Borealis. It is too faint to be visible to the naked eye with an apparent visual magnitude of 8.07. The star is located at a distance of 158 light years from the Sun based on parallax. Prior to the discovery of a companion, this served as an IAU radial velocity standard, and it is receding from the Sun at a rate of +37 km/s. The space velocity components of this star are (U, V, W) = (-21.77, -14.42, 1.67).
"Nichts bleibt für die Ewigkeit" is a song by Die Toten Hosen. It's the first single and the sixth track from the album Opium fürs Volk.
"Wünsch DIR was" is a song by Die Toten Hosen. It's the second single and the thirteenth track from the album Kauf MICH!.
"Alles aus Liebe" is a song by the German punk rock band Die Toten Hosen. It is the third single and the twelfth track from the album Kauf MICH!.
"Kauf MICH!" is a song by Die Toten Hosen. It's the fourth single and the seventh track from the album Kauf MICH!. The single cover is designed as a typical washing powder box.
SN 2005E was a calcium-rich supernova first observed in January 2005 that scientists concluded was a new type of cosmic explosion. The explosion originated in the galaxy NGC 1032, approximately 100 million light years away.
Hans Neleman is a Dutch-born international photographer and film director who lives in Connecticut and working in New York City. He is also the founder of boutique stock photography agency Win-initiative and its promotional magazine, WINk.
WIN-Initiative is an independent stock photography company that licenses images based on global youth culture. Founded in 2007 by photographer Hans Neleman, WIN, which stands for Worldwide Image Navigation, licenses images from its community of photographers from around the world. Essentially functioning as a collective, WIN Scouts are located in 22 countries. These Scouts assist in finding and retaining new talent, as well as being the liaison with the WIN headquarters team in SoHo, New York City.
Midostaurin, sold under the brand name Rydapt & Tauritmo both by Novartis, is a multi-targeted protein kinase inhibitor that has been investigated for the treatment of acute myeloid leukemia (AML), myelodysplastic syndrome (MDS) and advanced systemic mastocytosis. It is a semi-synthetic derivative of staurosporine, an alkaloid from the bacterium Streptomyces staurosporeus.
Willem Anton van Vloten is a Dutch dermatologist.
Tim Nelemans is a Dutch former professional footballer who played as a forward for Eerste Divisie club FC Oss. Nelemans also played for FC Eindhoven from 2001 to 2010.
Buttock cells are cells having a notched appearance that are found in certain malignancies, such as non-Hodgkin's lymphoma, mycosis fungoides, and Sézary syndrome.
NY Virginis is a binary star about 1,940 light-years away. The primary belongs to the rare class of subdwarf B stars, being former red giants with their hydrogen envelope completely stripped by a stellar companion. The companion is a red dwarf star. The binary nature of NY Virginis was first identified in 1998, and the extremely short orbital period of 0.101016 d, together with brightness variability on the timescale of 200 seconds was noticed, resulting in the identification of the primary star as a B-type subdwarf in 2003. Under a proposed classification scheme for hot subdwarfs it would be class sdB1VII:He1. This non-standard system indicates that it is a "normal" luminosity for a hot subdwarf and that the spectrum is dominated by hydrogen rather than helium.
GP Comae Berenices, abbreviated to GP Com and also known as G 61-29, is a star system composed of a white dwarf orbited by a planetary mass object, likely the highly eroded core of another white dwarf star. The white dwarf is slowly accreting material from its satellite at a rate of (3.5±0.5)×10−11 M☉/year and was proven to be a low-activity AM CVn star. The star system is showing signs of a high abundance of ionized nitrogen from the accretion disk around the primary.
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