mick laBriola

These excerpts are small sections from a new VLT Survey Telescope (VST) image of the Lagoon Nebula. This giant cloud of gas and dust is creating intensely bright young stars, and is home to young stellar clusters. These data form part of a huge treasure trove of publicly available images from the ESO survey telescopes.

The Lagoon Nebula (catalogued as Messier 8 or M8, NGC 6523, Sharpless 25, RCW 146, and Gum 72) is a giant interstellar cloud in the constellation Sagittarius. It is classified as an emission nebula and as an H II region.

The Lagoon Nebula was discovered by Giovanni Hodierna before 1654 and is one of only two star-forming nebulae faintly visible to the eye from mid-northern latitudes. Seen with binoculars, it appears as a distinct oval cloudlike patch with a definite core. Within the nebula is the open cluster NGC 6530.

The Lagoon Nebula is estimated to be between 4,000-6,000 light-years from the Earth. In the sky of Earth, it spans 90′ by 40′, which translates to an actual dimension of 110 by 50 light years. Like many nebulas, it appears pink in time-exposure color photos but is gray to the eye peering through binoculars or a telescope, human vision having poor color sensitivity at low light levels. The nebula contains a number of Bok globules(dark, collapsing clouds of protostellar material), the most prominent of which have been catalogued by E. E. Barnard as B88, B89 and B296. It also includes a funnel-like or tornado-like structure caused by a hot O-type star that emanates ultraviolet light, heating and ionizing gases on the surface of the nebula. The Lagoon Nebula also contains at its centre a structure known as the Hourglass Nebula (so named by John Herschel), which should not be confused with the better known Hourglass Nebula in the constellation of Musca. In 2006 the first four Herbig–Haro objects were detected within the Hourglass, also including HH 870. This provides the first direct evidence of active star formation by accretion within it.

Johnny “Big Moose” Walker (June 27, 1927 – November 27, 1999) was an American Chicago blues and electric blues pianist and organist. He worked with many blues musicians, including Ike Turner, Sonny Boy Williamson II, Lowell Fulson, Choker Campbell, Elmore James, Earl Hooker, Muddy Waters, Otis Spann, Sunnyland Slim, Jimmy Dawkins and Son Seals.^[2]

Walker was primarily a piano player but was also proficient on the electronic organ and the bass guitar (he played the bass guitar when backing Muddy Waters). He recorded solo albums and accompanied other musicians in concert and on recordings.

John Mayon Walker was born in the unincorporated community of Stoneville, Mississippi, partly of Native American ancestry. He acquired his best-known stage name in his childhood in Greenville, Mississippi, derived from his long, flowing hair. He learned to play several instruments, including the church organ, guitar, vibraphone and tuba.

St. Elmo Sylvester Hope (June 27, 1923 – May 19, 1967) was an American jazz pianist, composer, and arranger, chiefly in the bebop and hard bopgenres. He grew up playing and listening to jazz and classical music with Bud Powell, and both were close friends of another influential pianist, Thelonious Monk.

Hope survived being shot by police as a youth to become a New York-based musician who recorded with several emerging stars in the early to mid-1950s, including trumpeter Clifford Brown, and saxophonists John Coltrane, Lou Donaldson, Jackie McLean, and Sonny Rollins. A long-term heroin user, Hope had his license to perform in New York’s clubs withdrawn after a drug conviction, so he moved to Los Angeles in 1957. He was not happy during his four years on the West Coast, but had some successful collaborations there, including with saxophonist Harold Land.

More recordings as leader ensued following Hope’s return to New York, but they did little to gain him more public or critical attention. Further drug and health problems reduced the frequency of his public performances, which ended a year before his death, at the age of 43. He remains little known, despite, or because of, the individuality of his playing and composing, which were complex and stressed subtlety and variation rather than the virtuosity predominant in bebop.

Elmo Hope was born on June 27, 1923, in New York City. His parents, Simon and Gertrude Hope, were immigrants from the Caribbean, and had several children. Elmo began playing the piano aged seven. He had classical music lessons as a child, and won solo piano recital contests from 1938. Fellow pianist Bud Powell was a childhood friend; together, they played and listened to jazz and classical music. Hope attended Benjamin Franklin High School, which was known for its music program. He developed an excellent understanding of harmony, and composed jazz and classical pieces at school.

Lester Rallingston “Shad” Collins (June 27, 1910 – June 6, 1978) was an American jazz trumpet player, composer and arranger, who played in several leading bands between the 1930s and 1950s, including those led by Chick Webb, Benny Carter, Count Basie, Lester Young, Cab Calloway and Sam “The Man” Taylor.

Born in Elizabeth, New Jersey, the son of a clergyman, he acquired the nickname of “Shad” in his teens, and by the late 1920s had joined Charlie Dixon‘s band. He also performed with pianist Eddie White, before joining Chick Webb’s band in 1931. In the mid-1930s he played in Teddy Hill‘s band, with whom he toured in Britain and Europe, before joining the Count Basie Orchestra. He performed in Basie’s band at the From Spirituals to Swing concerts in New York City in 1938 and 1939. He also worked in the late 1930s in bands led by Benny Carter, Lester Young and Don Redman, among others.

Eleftheria Arvanitaki has been one of the most important figures of contemporary Greek music for the past years. The clarity and emotional depth of her voice, her magical stage presence, and the sincerity in her musical choices allow her to combine traditional Greek music idioms with up-to-date western rhythms and sounds.

The galaxy NGC 1187 is seen almost face-on, which gives us a good view of its spiral structure. About half a dozen prominent spiral arms can be seen, each containing large amounts of gas and dust. The bluish features in the spiral arms indicate the presence of young stars born out of clouds of interstellar gas.

Looking towards the central regions, we see the bulge of the galaxy glowing yellow. This part of the galaxy is mostly made up of old stars, gas and dust. In the case of NGC 1187, rather than a round bulge, there is a subtle central bar structure. Such bar features are thought to act as mechanisms that channel gas from the spiral arms to the centre, enhancing star formation there.

Around the outside of the galaxy many much fainter and more distant galaxies can also be seen. Some even shine right through the disc of NGC 1187 itself. Their mostly reddish hues contrast with the pale blue star clusters of the much closer object.

NGC 1187 looks tranquil and unchanging, but it has hosted two supernovae explosions since 1982. A supernova is a violent stellar explosion, resulting from the death of either a massive star or a white dwarf in a binary system . Supernovae are amongst the most energetic events in the Universe and are so bright that they often briefly outshine an entire galaxy before fading from view over several weeks or months. During this short period a supernova can radiate as much energy as the Sun is expected to emit over its entire life span.

In October 1982, the first supernova seen in NGC 1187 — SN 1982R was discovered at ESO’s La Silla Observatory and more recently, in 2007, the amateur astronomer Berto Monard in South Africa spotted another supernova in this galaxy — SN 2007Y. A team of astronomers subsequently performed a detailed study and monitored SN 2007Y for about a year using many different telescopes . This new image of NGC 1187 was created from observations taken as part of this study and the supernova can be seen, long after the time of maximum brightness, near the bottom of the image.

These data were acquired using the FORS1 instrument attached to the ESO’s Very Large Telescope at the Paranal Observatory in Chile.

Reginald “Reggie” Workman (born June 26, 1937 in Philadelphia, Pennsylvania) is an American avant-garde jazz and hard bop double bassist, recognized for his work with both John Coltrane and Art Blakey.

Workman was a member of jazz groups led by Gigi Gryce, Roy Haynes, Wayne Shorter and Red Garland. In 1961, Workman joined the John ColtraneQuartet, replacing Steve Davis. He was present for the saxophonist’s Live at the Village Vanguard sessions, and also recorded with a second bassist (Art Davis) on the 1961 album, Olé Coltrane. After a European tour, Workman left Coltrane’s group at the end of the year. Workman also played with James Moody, Art Blakey‘s Jazz Messengers, Yusef Lateef, Pharoah Sanders, Herbie Mann and Thelonious Monk. He has recorded with Archie Shepp, Lee Morgan and David Murray. Workman, with pianist Tommy Flanagan and drummer Joe Chambers, formed The Super Jazz Trio in 1978.

Big Bill Broonzy (born Lee Conley Bradley, June 26, 1903 – August 14, 1958) was an American blues singer, songwriter and guitarist. His career began in the 1920s, when he played country blues to mostly African-American audiences. Through the 1930s and 1940s he successfully navigated a transition in style to a more urban blues sound popular with working-class African-American audiences. In the 1950s a return to his traditional folk-blues roots made him one of the leading figures of the emerging American folk music revival and an international star. His long and varied career marks him as one of the key figures in the development of blues music in the 20th century.

Broonzy copyrighted more than 300 songs during his lifetime, including both adaptations of traditional folk songs and original blues songs. As a blues composer, he was unique in writing songs that reflected his rural-to-urban experiences.

Born Lee Conley Bradley, he was one of the seventeen children of Frank Broonzy (Bradley) and Mittie Belcher. The date and place of his birth are disputed. Broonzy claimed to have been born in Scott, Mississippi, but a body of emerging research compiled by the blues historian Robert Reisman suggests that he was born in Jefferson County, Arkansas.

The band’s catchy style is inspired by Afro-Colombian music, fueled by accordion and slow, steady cumbia beats along with vallenato rhythms.

Central region of the Trifid Nebula (M20 in the Messier Catalogue) taken by the Gemini North 8-meter Telescope on Mauna Kea on the Big Island of Hawaii, June 5, 2002. Located in the constellation of Sagittarius, the beautiful nebula is a much-photographed, dynamic cloud of gas and dust where stars are being born. One of the massive stars at the nebula’s center was born approximately 100,000 years ago. The nebula’s distance from the Solar System remains in dispute, but it is generally agreed to be somewhere between 2,200 to 9,000 light years away.

Joe Chambers (born June 25, 1942, near Philadelphia) is an American jazz drummer, pianist, vibraphonist and composer. He attended the Philadelphia Conservatory for one year. In the 1960s and 1970s Chambers gigged with many high-profile artists such as Eric Dolphy, Charles Mingus, Wayne Shorter, and Chick Corea. He has released eight albums as a bandleader and been a member of several incarnations of Max Roach‘s M’Boom percussion ensemble.

He has also taught, including at the New School for Jazz and Contemporary Music in New York City, where he leads the Outlaw Band.

Clifton Chenier (June 25, 1925 – December 12, 1987), a Louisiana French-speaking native of Opelousas, Louisiana, was an eminent performer and recording artist of Zydeco, which arose from Cajun and Creole music, with R&B, jazz, and blues influences. He played the accordion and won a Grammy Award in 1983. In 1984 he was honored as a National Heritage Fellow.^[3] He was inducted posthumously into the Blues Hall of Fame in 1989, and the Louisiana Music Hall of Fame in 2011. In 2014, he was a Grammy recipient of the Lifetime Achievement Award.

He was known as the King of Zydeco, and also billed as the King of the South.

John Henry Smith II (June 25, 1922 – June 11, 2013) was an American cool jazz and mainstream jazz guitarist. He wrote “Walk, Don’t Run” in 1954. In 1984, Smith was inducted into the Alabama Jazz Hall of Fame.

An extremely diverse musician, Johnny Smith was equally at home playing in the famous Birdland jazz club or sight-reading scores in the orchestral pit of the New York Philharmonic. From Schoenberg to Gershwin to originals, Smith was one of the most versatile guitarists of the 1950s.

As a staff studio guitarist and arranger for NBC from 1946 to 1951, and on a freelance basis thereafter until 1958, he played in a variety of settings from solo to full orchestra and had his own trio, The Playboys, with Mort Lindsey and Arlo Hults.

https://www.youtube.com/watch?v=oEJQETSaeMY

Haig Yazdjian was born of Armenian parents in Syria and has been living in Greece for the last 20 years. In Syria he discovered the enchanting elements of Eastern music, and took up the ud as the means to express an inner undiscovered domain.

https://www.youtube.com/watch?v=Wu59WhIN8rk

Your Community Band!
Performing Sunday 6-24-18 2pm
East Phillips Park (near Little Earth)
2307 17th Ave S, Minneapolis, MN 55404
An eclectic brass band extravaganza.
Ralph-tuba, Sawebone and Rob-trombone, Andrew-clarinet,Dana,Kathryn,Jill-flutes,Hilary-trumpet, mick-drums,
Russell-al s, Van-trombone
Performing this Abdullah Ibrahim Dollar Brand tune.

Approximately 95 million light-years away, in the southern constellation of Octans (The Octant), lies NGC 7098 — an intriguing spiral galaxy with numerous sets of double features. The first of NGC 7098’s double features is a duo of distinct ring-like structures that loop around the galaxy’s hazy heart. These are NGC 7098’s spiral arms, which have wound themselves around the galaxy’s luminous core. This central region hosts a second double feature: a double bar.

NGC 7098 has also developed features known as ansae, visible as small, bright streaks at each end of the central region. Ansae are visible areas of overdensity — they commonly take looping, linear, or circular shapes, and can be found at the extremities of planetary ring systems, in nebulous clouds, and, as is the case with NGC 7098, in parts of galaxies that are packed to the brim with stars.

This image is formed from data gathered by the FOcal Reducer and low dispersion Spectrograph (FORS) instrument, installed on ESO’s Very Large Telescope at Paranal Observatory. An array of distant galaxies are also visible throughout the frame, the most prominent being the small, edge-on, spiral galaxy visible to the left of NGC 7098, known as ESO 048-G007.