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Images of 'Haro' found, 72

Thirty Years War: “” Interview of the King of France Louis XIV (1638-1715) and Philip IV of Spain (1605-1665) on the island of Paisans on 7/11/1659”” Spain agrees to sign the Treaty of the Pyrenees. The daughter of Philip IV, Marie Therese (Marie-Therese) of Austria (1638-1683), future queen of France, behind the king of Spain. The trade negociators Cardinal Jules Mazarin (Giulio Raimondo Mazzarino or Mazarino) (1602-1661) and Luis de Haro (1598-1661) are present. Also represented are Anne of Austria (1601-1666), Jean Baptiste (Jean-Baptiste) Colbert (1619-1683), Antoine III of Gramont (1604-1678) and Philippe Duke of Orleans (1640-1701) dit Monsieur. Painting by Laumosnier (late 17th-early 18th century), oil on canvas, by Charles Le Brun and Adam Frans Van Der Meulen. French Art, 18th century. Musee de Tesse, Le Mans.
The Mourning of Countess de Haro, by Antonio Canova (1757-1822), marble relief, 186x220 cm, Detail, 1806-1808
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'Clameur de Haro, Guernsey', Arents Cigarette Card, c.1919-40 (colour litho)
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Southern Crown Nebula - The CRA reflection nebula - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. On the right, the globular cluster NGC 6723, located 30 000 light years from Earth in Sagittarius. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. Corona Australis (the southern crown, CRA) is in the far southern sky but visible from the southern states of the USA. The constellation is small but distinctive. The conspicuous globular cluster NGC 6723 is at the western (right) edge of the photograph, but it is in Sagittarius, and is about 30,000 light years distant. Almost all the nebulosity here is starlight, reflected from minute grains of dust, some of which gather into darker condensations ('molecular clouds'), blotting out the background stars. Fainter features can be seen here. Shiny NGC 6726 - 27 near middle of image contains both a visual binary and a variable star. Other wispy nebulae in the western part of the dark cloud betray the presence of young, hidden stars
PEACE OF THE PYRENEES 1659
Ara De Haro
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Ara De Haro
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Spain, Haro, Rioja vines
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Monument to Don Diego Lopez de Haro (1250-1310), 1890, Circular Square, Bilbao, Basque Country, Spain, 19th century
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Alcalde Francisco de Haro  (print)
Nebula NGC 7129 in Cephee - Reflection nebula NGC 7129 in Cepheus - Nebula by reflexion located 3300 years - light of the Earth. This nebula houses very young stars, aged less than a million years old. NGC 7129 is a star forming region located in Cepheus constellation, 3300 light years from us. Several Herbig Haro objects are visible in this nebula. Herbig - Haro objects are small emission nebulae found around young developing stars (protostars) and which are believed to be transient in their nature, for they only exist for a few thousand years
Francisco de Haro, c.1835 (engraving)
Southern Crown Nebula - The Corona Australis nebula (NGC 6726 - 27 - 29) - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. Image made with Siding Spring's 3.9m telescope. This spectacular reflection nebula is the result of a few bright stars caught up in a large, dusty cloud. If that is all there was here, this region would be considered to be like the Pleiades, an accidental association of dust and stars. However, there are features here that show the dark cloud to be an active star forming nebula, though most of the action is hidden from view. The peculiar yellowish curved streak near the two bright reflection nebulae surround an intriguing object best seen in infrared light, R CRA, a young star still accreting interstellar material on to its surface. It seems to be the source of two compact but distinctly red patches which are Herbig - Haro objects, often the first visible signs of star formation occurring deep inside dark clouds. These compact nebulae are ejected from proto - stars during the later stages of star formation and sometimes appear in pairs, moving in opposite directions from the hidden star forming region. The R CRA complex is about 500 light years distant, one of the nearest star - forming regions
Star births in the nebula NGC 6729 - Young stars in the nebula NGC 6729 - Close up on a star-forming region. The new stars are invisible, hidden behind the dust cloud at the top left of the image, but the material they eject at very high speed causes colorful and luminous arcs in contact with the surrounding gas. Image obtained in Chile with the VLT. This very detailed false - colour image from Eso's Very Large Telescope shows the dramatic effects of very young stars on the dust and gas from which they were born in the star - forming region NGC 6729. The baby stars are invisible in this picture, being hidden behind dust clouds at the upper left of the picture, but material they are ejecting is crashing into the surroundings at speeds of that can be as high as one million kilometres per hour. These shocks cause the gas to shine and create the strangely coloured glowing arcs and blobs known as Herbig - Haro objects. In this view the Herbig - Haro objects form two lines marking out the probable directions of ejected material. One stretches from the upper left to the lower centre, ending in the bright, circular group of glowing blobs and arcs at the lower centre. The other starts near the left upper edge of the picture and extends towards the centre right. The peculiar scimitar - shaped bright feature at the upper left is probably mostly due to starlight being reflected from dust and is not a Herbig - Haro object. This picture was taken by the FORS1 instrument and records the scene in the light of glowing hydrogen and sulphur
Nebula NGC 7129 in Cephee: Nebula by reflexion located 3300 light years from Earth. This nebula houses very young stars, aged less than a million years old. - NGC 7129 is a young compact star forming region which displays an unusual patchwork of colorful nebulosity and bright stars contrasted against the dust clouds of the Milky Way. NGC 7129 contains several bright reflection nebulae including the large blue reflection cloud NGC 7133 and the unusual small yellow reflection cloud LBN497. Also conspicuous in the field are several bright Herbig-Haro objects, the signatures of young stellar objects soon to emerge in the main sequence. The dominant blue reflection nebula, NGC 7133 is illuminated by two young B-type stars BD+65* 1637 and BD+65* 1638. Both stars are less than one million years old and represent the core of NGC 7129, a small cluster of low mass stars which populate the 36 light year wide cavity
Exoplanete near an object by Herbig - Haro - Artist's view
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7th Marqu?00730020del Carpio Haro y Guzm?006e0000
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Nebula of the cone NGC 2264 in the Unicorn - Nebulae in Monoceros - The nebula of the Cone below, is a region about 2600 years - light from the Earth. The bright star in the high center is S Monocerotis, a star of magnitude 4.7. Nests in these gas clouds, the Christmas tree, a cluster of young stars whose shape evokes a Christmas tree. This wide - field image of the Christmas Tree Cluster was taken at the National Science Foundation's 0.9 - meter telescope on Kitt Peak with the NOAO Mosaic CCD camera. Also known as NGC2264, it is an open cluster of stars embedded in a diffuse nebula. It is located in the constellation of Monoceros, the Unicorn. The image also contains two famous nebula. At the bottom center of the image is the Cone Nebula, and to the upper left is the Fox Fur Nebula. The bright star just above the center of the image is known as S Mon. The gentle arcs in orange and blue near the center of the image are Herbig Haro objects, jets of gas from protostars embedded in the nebula. This image was created by combining emission - line images in Hydrogen - alpha (red - orange), Oxygen [O III] (light blue) and Sulfur [S II] (blue - violet)
Sarcophagus of the Queen Dona Mencia Lopez de Haro (1223-1272)
7th Marqu?00730020del Carpio Haro y Guzm?006e0000
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Sepulcher of Dona Urraca López de Haro (1125-1262)
Nebula of the cone NGC 2264 and S star Monocerotis - NGC 2264 and S Monocerotis - Region H II located about 2600 years - light from Earth. The bright star is S Monocerotis, a star of magnitude 4.7. Image obtained by Siding Spring's 3.9m telescope. The region around the 4.7 magnitude star S Mon is a fascinating mixture of red fluorescent hydrogen and dark, obscuring dust lanes. Some dust patches are close enough to bright stars to reflect light from them; these appear blue for the same reason that the day - time sky is blue - because some of the interstellar particles preferentially scatter blue light. Some of the wispy tendrils of nebulosity are Herbig - Haro objects, jets of matter ejected from newly - formed stars still hidden within the nebula. About 250 stars have been recognised as members of NGC 2264 which is at a distance of about 2700 light years
Nebula of the cone NGC 2264 and S star Monocerotis - NGC 2264 and S Monocerotis - Region H II located about 2600 years - light from Earth. The bright star is S Monocerotis, a star of magnitude 4.7. Image obtained by Siding Spring's 3.9m telescope. The region around the 4.7 magnitude star S Mon is a fascinating mixture of red fluorescent hydrogen and dark, obscuring dust lanes. Some dust patches are close enough to bright stars to reflect light from them; these appear blue for the same reason that the day - time sky is blue - because some of the interstellar particles preferentially scatter blue light. Some of the wispy tendrils of nebulosity are Herbig - Haro objects, jets of matter ejected from newly - formed stars still hidden within the nebula. About 250 stars have been recognised as members of NGC 2264 which is at a distance of about 2700 light years
Pedro Fernández de Velasco, 2nd Count of Haro, after an etching in Retratos de Los Españoles Ilustres, Madrid, Spain, pub. 1791
Southern Crown Nebula - The tail of the CRA reflection nebula - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. On the right, the globular cluster NGC 6723, located 30 000 light years from Earth in Sagittarius. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. Corona Australis (the southern crown, CRA) is in the far southern sky but visible from the southern states of the USA. The constellation is small but distinctive. The conspicuous globular cluster NGC 6723 is at the western (right) edge of the photograph, but it is in Sagittarius, and is about 30,000 light years distant. Our picture is about 4.5 degrees across and the extremely faint Corona Australis nebula meanders along the Sgr - CRA border nebula in the same E - W direction. Almost all the nebulosity here is starlight, reflected from minute grains of dust, some of which gather into darker condensations ('molecular clouds'), blotting out the background stars. By far the largest and densest of the molecular clouds is at the western end of the picture, seen in more detail here. It is about a degree long, corresponding to eight light years at the 500ly distance of the nebula and is extremely opaque - - background stars are dimmed by an astonishing 35 magnitudes. However, not all is darkness, and the dusty cloud appears to be tipped by a pair of bright stars, embedded in bright reflection nebulae. The brightest of these is NGC 6726 - 27 and it contains both a visual binary and a variable star. Other wispy nebulae in the western part of the dark cloud betray the presence of young, hidden stars
Southern Crown Nebula - The Corona Australis nebula (NGC 6726 - 27 - 29) - R Coronae Australis is one of the closest and most intense star-forming regions; visible in the southern hemisphere, it is located about 500 years from Earth. R Coronae Australis is the star in the center of the image that illuminates a reddish nebula around it. Image obtained in Chile at the observatory of La Silla with the 2.2 meter MPG/ESO telescope. Image of R Coronae Australis region in the southern Milky Way, obtained with the Wide Field Imager (WFI) (camera) at the 2.2 - m MPG/ESO Telescope on La Silla (Chile). The R Coronae Australis complex of young stars and interstellar gas clouds is one of the nearest star - forming regions, at a distance of approx. 500 light - years from the Sun. It is seen in the southern constellation of that name (The “Southern Crown”). R Coronae Australis, the bright star from which the entire complex is named, is located at the center of the field and illuminates the reddish nebula around it. The bright star in the lower part, illuminating a somewhat bluer nebula, is known as TY Coronae Australis. The brightness of these two stars and several others in the same field is variable. They belong to the so - called “” T Tauri””” class, a type that is quite common in star - forming regions. T Tauri stars are in the early stages of stellar evolution and display various observable characteristics of this phase, e.g. emission at visible and infrared wavelengths due to the accretion of matter left over from their formation, as well as X - ray emission. The nebulosity seen in this picture is mostly due to reflection of the stellar light by small dust particles. The stars in the R Coronae Australis complex do not emit sufficient ultraviolet light to ionize a substantial fraction of the surrounding hydrogen, and thus cause this gas to glow. Also visible are so - called Herbig - Haro objects, dense clumps of gas ejected f
Cartoon on the wine crisis in France in 1907. Haro on the clear water drinker. Cover of the little Journal.
FINNISH SWIMMERS SEPPALA,PIHLAVA AND HARO IN FUKUOKA FOR WORLD SWIMMING
CHAMPIONSHIPS, 2001-07-19 (photo)
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Mourning of Countess de Haro by Antonio Canova (1757-1822), marble relief, 186x220 cm, 1806-1808
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Don Luis Mendez de Haro (1598-1661) near the Ile des Faisans (w/c on paper)
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The Mourning of Countess de Haro by Antonio Canova (1757-1822), marble relief, 186x220 cm, detail, 1806-1808
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The Mourning of Countess de Haro by Antonio Canova (1757-1822), marble relief, 186x220 cm, detail, 1806-1808
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CUBAN FELIX SAVON BOXES DURING CARIBBEAN GAMES IN MARACAIBO, 1998-08-20 (photo)
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CUBA VS MEXICO BOXING ACTION AT THE CARIBBEAN GAMES, 1998-08-20 (photo)
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Dark Nebula LDN 673 in Aquarius - LDN 673 dark nebula in Aquila - This telescopic close - up looks towards the region at a fragmented Aquila dark cloud complex identified as LDN 673, stretching across a field of view slightly wider than the full moon. In the scene, visible indications of energetic outflows associated with young stars include the small red tinted nebulosity RNO 109 at top left and Herbig - Haro object HH32 above and right of center. The dark clouds in Aquila are estimated to be some 600 light - years away
Albinia Gibbs, 1876
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William Gibbs, 1872
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SPANISH POLICE PATROL THE STREETS OF MANCHESTER, 1997-02-26 (photo)
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Thirty Years War: “” Interview of the King of France Louis XIV (1638-1715) and Philip IV of Spain (1605-1665) on the island of Paisans on 7/11/1659”” Spain agrees to sign the Treaty of the Pyrenees. The daughter of Philip IV, Marie Therese (Marie-Therese) of Austria (1638-1683), future queen of France, behind the king of Spain. The trade negociators Cardinal Jules Mazarin (Giulio Raimondo Mazzarino or Mazarino) (1602-1661) and Luis de Haro (1598-1661) are present. Also represented are Anne of Austria (1601-1666), Jean Baptiste (Jean-Baptiste) Colbert (1619-1683), Antoine III of Gramont (1604-1678) and Philippe Duke of Orleans (1640-1701) dit Monsieur. From ap. tapestry, cardboard of Lebrun, “” 17th century - Institutions: usages et costumes, France 1590-1700” by Paul Lacroix, 1880.
Cometary Globula CG30 in the Stern - Cometary Globule CG30 - Cometary cells are small clouds of isolated gases. These, called CG30/31/38, are located about 1300 light years ago in the constellation Pupus. The Cometary Globules CG 30/31/38 are located 1300 light years away in Vela/Puppis constellations; they appear as finger - like extensions extending out in different directions. Bright rimmed globules and their more evolved cousin the cometary globule represent fascinating dynamic structures formed by the interplay of cold molecular clouds and hot ionizing stars. Typically the head of the globule faces a hot O - type star. The blood cells are known to be the birthplace of low mass stars. The globule head of CG 30 contains the Herbig Haro object HH 120, which is the outflow signature of a pre - main sequence star
Nebula NGC 6726 - 27 - 29 in the Southern Crown - The Corona Australis nebula (NGC 6726 - 27 - 29) Image of R Coronae Australis region in the southern Milky Way, obtained with the Wide Field Imager (WFI) (camera) at the 2.2 - m MPG/ESO Telescope on La Silla (Chile). The sky field shown measures approx. 33.7 x 31.9 arcmin2 (about the diameter of the full moon). The R Coronae Australis complex of young stars and interstellar gas clouds is one of the nearest star - forming regions, at a distance of approx. 500 light - years from the Sun. It is seen in the southern constellation of that name (The “Southern Crown”). R Coronae Australis, the bright star from which the entire complex is named, is located at the center of the field and illuminates the reddish nebula around it. The bright star in the lower part, illuminating a somewhat bluer nebula, is known as TY Coronae Australis. The brightness of these two stars and several others in the same field is variable. They belong to the so - called “” T Tauri””” class, a type that is quite common in star - forming regions. T Tauri stars are in the early stages of stellar evolution and display various observable characteristics of this phase, e.g. emission at visible and infrared wavelengths due to the accretion of matter left over from their formation, as well as X - ray emission. The nebulosity seen in this picture is mostly due to reflection of the stellar light by small dust particles. The stars in the R Coronae Australis complex do not emit sufficient ultraviolet light to ionize a substantial fraction of the surrounding hydrogen, and thus cause this gas to glow. Also visible are so - called Herbig - Haro objects, i.e., dense clumps of gas ejected from the immediate vicinity of newly formed stars with velocities of about 200 km/sec. The observations were obtained on the night of 30 August 2000
Perseus Molecular Cloud, 2015 (digital photo)
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Variable star PV Cephei and nebula Gyulbudagyan - Variable star PV Cephei with Gyulbudagyan's nebula - PV Cephei is an excessively fast variable star, moving almost 20 km per second in the interstellar medium. This young star, formed about 500,000 years ago, is now more than 30 years ago - light from its birthplace, the cluster of stars of the Iris nebula, NGC 7023. PV Cephei is the small orange star with a gas cloud located in the upper left middle of the image. Image obtained on October 19, 2008 with a telescope measuring 61 cm in diameter. PV Cephei is a variable star moving at roughly 20 km/sec through the interstellar medium. This young star was formed about 500,000 years ago and is located now at about 30 light years from its birth place, the star cluster of Iris nebula (NGC 7023). PV Cephei is the small oranged star visible near the middle of the image, at right of the brilliant blue star. It is associated with a small cloud of gas. Image taken on October 19 2008 with a 24 - inch telescope
BUILDERS WORK AT THE JEWISH SETTLEMENT OUTPOST MAALE HAROE NEAR TO THE WEST BANK CITY OF NABLUS, 2003-07-28 (photo)
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Movie directors (L-R) Oliver Hirschbiegel from Germany, Abderrahmane Sissako from Mauretania, Klaus Haeroe from Finland and German-Afghan director and script author Burhan Qurbani celebrate together after receiving their trophies of the Peace Award of the German Movie following a ceremony at the Cuvillies Theater in Munich, Germany, 02 July 2015 (photo)
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