Antoinette De Vaucouleurs
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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. In addition to ongoing collaborations with her husband, Gérard de Vaucouleurs, she carried out her own research in
spectroscopy Spectroscopy is the field of study that measures and interprets the electromagnetic spectra that result from the interaction between electromagnetic radiation and matter as a function of the wavelength or frequency of the radiation. Matter wa ...
. Her contributions (and Gérard's) were recognized in a '' festschrift'' in 1988, entitled ''The World of Galaxies''.


Early life and education

Antoinette Piétra was born on November 14, 1921, in Paris, France. She married Gérard de Vaucouleurs on October 31, 1944. De Vaucouleurs studied mathematics, physics, and astronomy at the Sorbonne from 1944 to 1948.


Career

De Vaucouleurs worked as a laboratory spectroscopist at the
Institut d'Astrophysique de Paris The Institut d'Astrophysique de Paris (translated: Paris Institute of Astrophysics) is a research institute in Paris, France. The Institute is part of the Sorbonne University and is associated with the CNRS Centre national de la recherche scientifiq ...
from 1948 to 1949. From 1950 to 1951, she acted as a voluntary assistant at the
University of London Observatory UCL Observatory (called the University of London Observatory until 2015) at Mill Hill in London is an astronomical teaching observatory. It is part of the Department of Physics and Astronomy at University College London. History The Observator ...
(ULO)'s Mill Hill Observatory. There she measured spectra from the 24-inch Wilson reflector, a gift to the observatory from J. G. Wilson in 1925. De Vaucouleurs moved to
Canberra, Australia Canberra ( ) is the capital city of Australia. Founded following the federation of the colonies of Australia as the seat of government for the new nation, it is Australia's largest inland city and the eighth-largest city overall. The c ...
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. In 1957, the de Vaucouleurs were invited to
Lowell Observatory Lowell Observatory is an astronomical observatory in Flagstaff, Arizona, United States. Lowell Observatory was established in 1894, placing it among the oldest observatories in the United States, and was designated a National Historic Landmark ...
in
Flagstaff, Arizona Flagstaff ( ) is a city in, and the county seat of, Coconino County, Arizona, Coconino County in northern Arizona, in the southwestern United States. In 2019, the city's estimated population was 75,038. Flagstaff's combined metropolitan area has ...
. In 1958 they moved to the
Harvard Observatory The Harvard College Observatory (HCO) is an institution managing a complex of buildings and multiple instruments used for astronomical research by the Harvard University Department of Astronomy. It is located in Cambridge, Massachusetts, United St ...
in Cambridge, Massachusetts, where they remained from 1958 to 1960. 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. In 1962, de Vaucouleurs became a naturalized American citizen.


Research

During her time in Paris, de Vaucouleurs discovered new spectroscopic doublets and perturbations in the secondary series of the infrared spectrum of potassium. She and Gérard used the Chalonge microphotometer to study the surface photometry of galaxies, leading to the formulation of "
De Vaucouleurs's law de Vaucouleurs's law, also known as the de Vaucouleurs profile or de Vaucouleurs model, describes how the surface brightness I of an elliptical galaxy varies as a function of apparent distance R from the center of the galaxy: : \ln I(R) = \ln I_ - ...
" for the surface brightness of an elliptical galaxy in 1948. In Australia, de Vaucouleurs worked first on Greenwich-style spectrophotometric gradients in the continua of southern bright stars and of the planet Mars. 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. She later published a photometry catalogue of galaxies with Giuseppe Longo (1983). 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. 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. 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 Struve reflector. She took over much of the tedious and painstaking work of reducing the data from the observation runs. De Vaucouleurs was a partner in her husband's early studies of the dimensions and structure of the
Large Magellanic Cloud The Large Magellanic Cloud (LMC), or Nubecula Major, is a satellite galaxy of the Milky Way. At a distance of around 50 kiloparsecs (≈160,000  light-years), the LMC is the second- or third-closest galaxy to the Milky Way, after the ...
, including the first quantitative analysis of the spectral composition of a galaxy from its spectrum. They used the strength of its absorption lines to determine the stellar population of the bar of the Large Magellanic Cloud. For fifteen years, Antoinette and Gerard de Vaucouleurs compiled and systematized the '' Reference Catalogue of Bright Galaxies'' (RCBG), one of the major catalogues of galaxies to be published after 1960. 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. 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. In addition, the ''Southern Galaxy Catalogue'' (1985) was completed by Harold Corwin with lesser levels of help from Antoinette and Gérard de Vaucouleurs. Throughout this work, de Vaucouleurs was well known for her attention to and memory for detail and her ability to discover and correct errors. The de Vaucouleurs are also known for their pioneering work on
superclusters A supercluster is a large group of smaller galaxy clusters or galaxy groups; they are among the largest known structures in the universe. The Milky Way is part of the Local Group galaxy group (which contains more than 54 galaxies), which in turn ...
. 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 In the 1950s the astronomer Gérard de Vaucouleurs recognized the existence of a flattened “local supercluster” from the Shapley-Ames Catalog in the environment of the Milky Way. He noticed that when one plots nearby galaxies in 3D, they lie mo ...
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 In physics, a redshift is an increase in the wavelength, and corresponding decrease in the frequency and photon energy, of electromagnetic radiation (such as light). The opposite change, a decrease in wavelength and simultaneous increase in f ...
movement. De Vaucouleurs passed away of
Bone-marrow cancer Multiple myeloma (MM), also known as plasma cell myeloma and simply myeloma, is a cancer of plasma cells, a type of white blood cell that normally produces antibody, antibodies. Often, no symptoms are noticed initially. As it progresses, bone p ...
on August 29, 1987. She continued to work until 10 weeks before her death.


Recognition

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".


Publications

* * * * *


External links

* Photograph of Antoinette de Vaucouleurs in


References

{{DEFAULTSORT:Vaucouleurs, Antoinette de 1921 births 1987 deaths University of Paris alumni French emigrants to the United States University of Texas at Austin faculty Scientists from Paris 20th-century American astronomers 20th-century French astronomers Women astronomers 20th-century women scientists