Antoinette de Vaucouleurs | |
---|---|
Born | Antoinette Piétra November 14, 1921 |
Died | August 27, 1987 65) | (aged
Alma mater | Sorbonne |
Scientific career | |
Fields | Astronomy |
Institutions | University of Texas at Austin |
Antoinette de Vaucouleurs (November 14, 1921, Paris, France-August 29, 1987, Austin, Texas, USA) was an astronomer who worked in the Astronomy Department of the University of Texas at Austin for 25 years (1961-1986) when few women worked in the field. [1] [2] In addition to ongoing collaborations with her husband, [3] Gérard de Vaucouleurs, she carried out her own research in spectroscopy. Her contributions (and Gérard's) were recognized in a festschrift in 1988, entitled The World of Galaxies. [4] [5]
Antoinette Piétra was born on November 14, 1921, in Paris, France. She married Gérard de Vaucouleurs on October 31, 1944. [1] [2] [6]
De Vaucouleurs studied mathematics, physics, and astronomy at the Sorbonne from 1944 to 1948. [1]
De Vaucouleurs worked as a laboratory spectroscopist at the Institut d'Astrophysique de Paris from 1948 to 1949. [1]
From 1950 to 1951, she acted as a voluntary assistant at the University of London Observatory (ULO)'s Mill Hill Observatory. [1] There she measured spectra from the 24-inch Wilson reflector, [7] a gift to the observatory from J. G. Wilson in 1925. [8]
De Vaucouleurs moved to Canberra, Australia in 1951, where she worked as an assistant to Richard Woolley, director of the Commonwealth Observatory at Mount Stromlo. During this time, she worked on the spectrophotometry of southern bright stars and of the planet Mars. [1]
In 1957, the de Vaucouleurs were invited to Lowell Observatory in Flagstaff, Arizona. [1] In 1958 they moved to the Harvard Observatory in Cambridge, Massachusetts, where they remained from 1958 to 1960. [2] [1]
In 1960, the de Vaucouleurs moved to the University of Texas at Austin which was forming a Department of Astronomy. There de Vaucouleurs held an official position as a Research Scientist Associate from 1961 to 1986 and was able to work with the McDonald Observatory. She also served on the Chancellor's Council of the University of Texas from 1980 onwards. [2]
In 1962, de Vaucouleurs became a naturalized American citizen. [2]
During her time in Paris, de Vaucouleurs discovered new spectroscopic doublets and perturbations in the secondary series of the infrared spectrum of potassium. [2] She and Gérard used the Chalonge microphotometer to study the surface photometry of galaxies, leading to the formulation of "De Vaucouleurs's law" for the surface brightness of an elliptical galaxy in 1948. [9]
In Australia, de Vaucouleurs worked first on Greenwich-style spectrophotometric gradients in the continua of southern bright stars and of the planet Mars. [2] She and Gérard were the first to take Harold Johnson's UBV photometric system for classifying stars according to their color and magnitude, and adapt it to the photoelectric-photometry of galaxies. [1] She later published a photometry catalogue of galaxies with Giuseppe Longo (1983). [10]
In 1957, De Vaucouleurs submitted her work on Spectral Types and Luminosities of B, A and F Southern Stars to the Royal Astronomical Society in London. It was the first quantitative spectral and luminosity classification of the 366 stars of the Morgan-Keenan system. It was considered one of the best classifications for MK types of southern stars. [2] [11]
De Vaucouleurs reportedly noticed variability in the centers of some Seyfert galaxies in 1958, but was discouraged from following up on the idea by her husband. Her suspicions were later confirmed by the discoveries of others. [12]
De Vaucouleurs was an active participant in her husband's extragalactic research. Between 1960 and 1978 she helped with the radial velocity surveys done at the McDonald Observatory using the 82 inches (2.1 m) Struve reflector. [1] [2] She took over much of the tedious and painstaking work of reducing the data from the observation runs. [5]
De Vaucouleurs was a partner in her husband's early studies of the dimensions and structure of the Large Magellanic Cloud, including the first quantitative analysis of the spectral composition of a galaxy from its spectrum. [5] They used the strength of its absorption lines to determine the stellar population of the bar of the Large Magellanic Cloud. [2] [13] [14]
For fifteen years, Antoinette and Gerard de Vaucouleurs compiled and systematized the Reference Catalogue of Bright Galaxies (RCBG), [15] one of the major catalogues of galaxies to be published after 1960. [16] It built upon the work of Harlow Shapley and Adelaide Ames in the Shapley-Ames Catalogue of Bright Galaxies and of others. The first Reference Catalogue was published in 1964. [17] It contained 2,599 objects, double the size of the original Shapley-Ames catalogue. The Second Reference Catalogue of Bright Galaxies (RC2), published by the de Vaucouleurs and Harold G. Corwin, Jr. in 1976, included 4,364 objects and considerably expanded the data provided about them. The Third Reference Catalogue of Bright Galaxies (RC3) included 23,022 objects, from a database of 73,197 galaxies at Lyons Observatory. [18] In addition, the Southern Galaxy Catalogue (1985) was completed by Harold Corwin with lesser levels of help from Antoinette and Gérard de Vaucouleurs. [19] [20] Throughout this work, de Vaucouleurs was well known for her attention to and memory for detail and her ability to discover and correct errors. [21]
The de Vaucouleurs are also known for their pioneering work on superclusters. [22] [23] [9] In 1953, on the basis of their joint work, Gerard put forth the controversial claim that the Milky Way was in fact part of a larger flattened system of galaxies since known as the Local Supercluster, They developed a supergalactic coordinate system based on the orientation of the Local Superclustor and other clusters, which has been used extensively to describe the distribution of nearby galaxies. De Vaucouleurs was active in studying galaxy redshift movement. [9]
De Vaucouleurs died of bone marrow cancer on August 29, 1987. She continued to work until 10 weeks before her death. [1]
The University of Texas at Austin established the Antoinette de Vaucouleurs Memorial Lectureship and Medal to be awarded annually to "an outstanding astronomer in recognition of a lifetime of dedication to astronomy". [1] [24]
Sandra Moore Faber is an American astrophysicist known for her research on the evolution of galaxies. She is the University Professor of Astronomy and Astrophysics at the University of California, Santa Cruz, and works at the Lick Observatory. She has made discoveries linking the brightness of galaxies to the speed of stars within them and was the co-discoverer of the Faber–Jackson relation. Faber was also instrumental in designing the Keck telescopes in Hawaii.
The Pinwheel Galaxy is a face-on, unbarred, and counterclockwise spiral galaxy located 21 million light-years from Earth in the constellation Ursa Major. It was discovered by Pierre Méchain in 1781 and was communicated that year to Charles Messier, who verified its position for inclusion in the Messier Catalogue as one of its final entries.
Messier 83 or M83, also known as the Southern Pinwheel Galaxy and NGC 5236, is a barred spiral galaxy approximately 15 million light-years away in the constellation borders of Hydra and Centaurus. Nicolas-Louis de Lacaille discovered M83 on 17 February 1752 at the Cape of Good Hope. Charles Messier added it to his catalogue of nebulous objects in March 1781.
Gérard Henri de Vaucouleurs was a French astronomer best known for his studies of galaxies.
Messier 81 (also known as NGC 3031 or Bode's Galaxy) is a grand design spiral galaxy about 12 million light-years away in the constellation Ursa Major. It has a D25 isophotal diameter of 29.44 kiloparsecs (96,000 light-years). Because of its relative proximity to the Milky Way galaxy, large size, and active galactic nucleus (which harbors a 70 million M☉ supermassive black hole), Messier 81 has been studied extensively by professional astronomers. The galaxy's large size and relatively high brightness also makes it a popular target for amateur astronomers. In late February 2022, astronomers reported that M81 may be the source of FRB 20200120E, a repeating fast radio burst.
Galaxy morphological classification is a system used by astronomers to divide galaxies into groups based on their visual appearance. There are several schemes in use by which galaxies can be classified according to their morphologies, the most famous being the Hubble sequence, devised by Edwin Hubble and later expanded by Gérard de Vaucouleurs and Allan Sandage. However, galaxy classification and morphology are now largely done using computational methods and physical morphology.
NGC 5866 is a lenticular galaxy in the constellation Draco. NGC 5866 was most likely discovered by Pierre Méchain or Charles Messier in 1781, and independently found by William Herschel in 1788. Measured orbital velocities of its globular cluster system imply that dark matter makes up only 34%±45% of the mass within 5 effective radii, a notable paucity.
NGC 6946, sometimes referred to as the Fireworks Galaxy, is a face-on intermediate spiral galaxy with a small bright nucleus, whose location in the sky straddles the boundary between the northern constellations of Cepheus and Cygnus. Its distance from Earth is about 25.2 million light-years or 7.72 megaparsecs, similar to the distance of M101 in the constellation Ursa Major. Both were once considered to be part of the Local Group, but are now known to be among the dozen bright spiral galaxies near the Milky Way but beyond the confines of the Local Group. NGC 6946 lies within the Virgo Supercluster.
The Astronomical Observatory of Belogradchik or Belogradchik Observatory is an astronomical observatory owned and operated by the Institute of Astronomy of the Bulgarian Academy of Sciences. It is located near the town of Belogradchik in northwestern Bulgaria, at the foot of the Western Balkan Mountains. The other observatory operated by the same institute is the Rozhen Observatory.
NGC 5820 is a lenticular galaxy in the constellation Boötes. It lies near NGC 5821, a galaxy with a similar mass at the same redshift.
NGC 5755 is a barred spiral galaxy in the constellation Boötes, member of Arp 297 interacting galaxies group of four: NGC 5752, NGC 5753, NGC 5754, and NGC 5755.
Adelaide Ames was an American astronomer and research assistant at Harvard University. She was best known for her work on detailed surveys of the brightest extra-galactic spiral nebulae. She contributed to the study of galaxies with her co-authorship of A Survey of the External Galaxies Brighter Than the Thirteenth Magnitude, which was later known as the Shapley-Ames catalog. Ames was a member of the American Astronomical Society. She was a contemporary of Cecilia Payne-Gaposchkin and her closest friend at the observatory.
IC 2560 is a spiral galaxy lying over 110 million light-years away from Earth in the constellation of Antlia. It was discovered by Lewis Swift in 1897.
NGC 7130 is a spiral galaxy located in the constellation Piscis Austrinus. It is located at a distance of about 220 million light years from Earth, which, given its apparent dimensions, means that NGC 7130 is about 100,000 light years across. It was discovered by John Herschel on September 25, 1834, and discovered independently by Lewis Swift on September 17, 1897. The location of the galaxy given in the New General Catalogue was off by 30 arcminutes in declination from the location of the galaxy.
NGC 5982 is an elliptical galaxy located in the constellation Draco. It is located at a distance of circa 130 million light years from Earth, which, given its apparent dimensions, means that NGC 5982 is about 100,000 light years across. It was discovered by William Herschel on May 25, 1788.
IC 5201 is a barred spiral galaxy located in the constellation Grus. It is located at a distance of about 35 million light years from Earth, which, given its apparent dimensions, means that IC 5201 is about 90,000 light years across. It was discovered by Joseph Lunt in 1900.
NGC 3729 is a barred spiral galaxy located in the constellation Ursa Major. It is located at a distance of circa 65 million light years from Earth, which, given its apparent dimensions, means that NGC 3729 is about 60,000 light years across. It was discovered by William Herschel on April 12, 1789.
NGC 4561 is a barred spiral galaxy in the constellation Coma Berenices. It was discovered by German-British astronomer William Herschel on April 13, 1784. This galaxy is located at a distance of 82 ± 14 million light-years (25.2 ± 4.3 Mpc) from the Milky Way, and is a member of the Virgo Cluster of galaxies. It is 13th magnitude with an angular size of 1.5′.
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