Such items recall the California journalist who reported an accident involving a movie star: `` The area in which Miss N -- was injured is spectacularly scenic ''.

Holmes went to Atlanta's Morehouse ( Negro ) College, where he is a B student and star halfback.

Because of its simplicity, star hopping is a very common method for finding objects that are close to naked-eye stars.

It is common for local societies to hold regular meetings, which may include activities such as star parties or presentations.

Aquarius is identified as " The Great One " in the Babylonian star catalogues and represents the god Ea himself, who is commonly depicted holding an overflowing vase.

The main feature of the family is the composite flower type in the form of capitula surrounded by involucral bracts. The name " Asteraceae " comes from Aster, the most prominent generum in the family, that derives from the Greek ἀστήρ meaning star, and is connected with its inflorescence star form.

The Latin name ' Asteraceae ' is derived from the type genus Aster, which is a Greek term, meaning " star ".

The history of astrometry is linked to the history of star catalogues, which gave astronomers reference points for objects in the sky so they could track their movements.

The observations show that the cloud is asymmetrical and matches the pattern of X-ray binaries ( binary star systems containing black holes or neutron stars ), mostly on one side of the galactic center.

* A smaller figure, next to the man, sitting on a chair ; as it is near the pole star, it may be seen by observers in the Northern Hemisphere through the whole year, although sometimes upside down ( the constellation Cassiopeia )

* α Antliae is the constellation's brightest star at magnitude 4. 25.

* δ Antliae is a blue double star 481 light years away.

* ζ Antliae is a wide double star 373 light years away.

The primary ( ζ < sup > 1 </ sup > Ant ) is of magnitude 5. 8, though it is a double star with a primary of magnitude 6. 2 and a secondary of magnitude 7. 0.

* δ Apodis is a double star with a separation of 103 arcseconds.

δ < sup > 1 </ sup > is a red giant star located 765 light years away, with a magnitude of 4. 7. δ < sup > 2 </ sup > is an orange giant star located 663 light years away, with a magnitude of 5. 3.

Among some amateur astronomers, NGC 246 has garnered the nickname " Pac-Man Nebula " because of the arrangement of its central stars and the surrounding star field.

It has an overall magnitude of 8. 0 and a central star of magnitude 11. 0 ; it is 2600 light-years from Earth.

The light from the central star was blanked out by a vector vortex coronagraph.

The central blob is noise left over after light from the star has been largely removed.

Its central star is of magnitude 11. 4, an unusually bright specimen.

As co-director, lead star and choreographer, Kelly was the central driving force.

The black central circle is produced by the camera's coronagraph, which hides the central star to allow the much fainter disks to be seen.

The hottest region, closest to the central star, appears blue because of emission from helium.

The central star itself is a white dwarf with a temperature of 120, 000 degrees Kelvin.

When it was pointed out to Niven that the Ringworld was dynamically unstable, in that once the center of rotation drifted away from the central sun, gravity would pull the ring into contact with the star, he used this as a plot element in the sequel novel, The Ringworld Engineers.

With his roles in Leone's films, Van Cleef became a major star of Spaghetti Westerns, playing central roles in films such as Death Rides a Horse, Day of Anger, The Big Gundown and The Sabata Trilogy.

The PPN is energized by the central star, causing it to emit strong infrared radiation and become a reflection nebula.

Collaminated stellar winds from the central star shape and shock the shell into an axially symmetric form, while producing a fast moving molecular wind .< ref name = mnras360_1 > The exact point when a PPN becomes a planetary nebula ( PN ) is defined by the temperature of the central star.

The PPN phase continues until the central star reaches a temperature of 30, 000 K, after which is it hot enough to ionize the surrounding gas.

The badge of the Presidential Medal of Freedom is in the form of a golden star with white enamel, with a red enamel pentagon behind it ; the central disc bears thirteen gold stars on a blue enamel background ( taken from the Great Seal of the United States ) within a golden ring.

A special grade of the medal, known as the Presidential Medal of Freedom with Distinction, has a larger execution of the same medal design worn as a star on the left chest along with a sash over the right shoulder, with its rosette ( blue with white edge, bearing the central disc of the medal at its center ) resting on the left hip.

Although both planets orbit their central star ( as depicted in Star Trek Nemesis ), Romulus and Remus are often referred to as a double planet.

With the high infrared energy input from the central star, ideal conditions are formed in these circumstellar envelopes for maser excitation.

In its simplest form, a star network consists of one central switch, hub or computer, which acts as a conduit to transmit messages.

An active star network has an active central node that usually has the means to prevent echo-related problems.

The star topology reduces the chance of network failure by connecting all of the systems to a central node.

The compact object that was created after the explosion lies in the center of the Crab Nebula and is a neutron star.

The Crab Nebula, the shattered remnants of a star which exploded as a supernova, the light of which reached Earth in 1054 AD

The Crab Nebula is a remnant of an exploded star.

At the center of the nebula lies the Crab Pulsar, a neutron star ( or spinning ball of neutrons ), 28 – 30 km across, which emits pulses of radiation from gamma rays to radio waves with a spin rate of 30. 2 times per second.

At the centre of the Crab Nebula are two faint stars, one of which is the star responsible for the existence of the nebula.

Image: The Crab Nebula-A Flickering X-ray Candle. ogv | Data from orbiting observatories show unexpected variations in the Crab Nebula's X-ray output, likely tied to the environment around its central neutron star.

Theoretical models of supernova explosions suggest that the star that exploded to produce the Crab Nebula must have had a mass of between 9 and 11 M < sub >☉</ sub >.

Stars with masses lower than 8 solar masses are thought to be too small to produce supernova explosions, and end their lives by producing a planetary nebula instead, while a star heavier than 12 solar masses would have produced a nebula with a different chemical composition to that observed in the Crab.

A significant problem in studies of the Crab Nebula is that the combined mass of the nebula and the pulsar add up to considerably less than the predicted mass of the progenitor star, and the question of where the ' missing mass ' is remains unresolved.

The Crab Pulsar ( PSR B0531 + 21 ) is a relatively young neutron star.

* The supernova of Beta Niobe at the end is interpreted quite differently by showing the star becoming a Crab Nebula-like nova and Sarpeidon's breaking up and being destroyed as the Enterprise warps away.

** Crab Pulsar, the central star in the Crab Nebula

The supernova that created the Crab Nebula observed in 1054, now known as the SN 1054, is an example of a guest star observed by Chinese astronomers, recorded also by the Arab astronomers, although it was not recorded by their European contemporaries.

* 1054-July 4, Chinese astronomers noted the appearance of a guest star, the supernova now called the Crab Nebula, Messier's M1.

The Crab Nebula is a remnant of an exploded star.

In 1942, Jan Oort, convinced that the Crab Nebula was the " guest star " of 1054 described by the Chinese, asked sinologist J. J. L.

The location of the guest star can in principle be deducted from the statement “ to the south-east of Tianguan, perhaps several inches away “, which for a long time perplexed modern astronomers, because if Tianguan is almost universally regarded as a correspondent for the star Zeta Tauri ( ζ Tauri ), the Crab nebula, following a clearly old explosion of stars about 1000 years ago, and therefore a natural candidate for this guest star, is not situated in the south-east but to the north-west of this star ( see the General localisation of the Event section below ).

If we centre the research on the star ζ Tauri, there is a remnant located in the immediate proximity: the Crab Nebula.