HOME

TheInfoList



OR:

George Howard Herbig (January 2, 1920 – October 12, 2013) was an American
astronomer An astronomer is a scientist in the field of astronomy who focuses their studies on a specific question or field outside the scope of Earth. They observe astronomical objects such as stars, planets, natural satellite, moons, comets and galaxy, g ...
at the
University of Hawaii A university () is an institution of higher (or tertiary) education and research which awards academic degrees in several academic disciplines. Universities typically offer both undergraduate and postgraduate programs. In the United States, th ...
Institute for Astronomy. He is perhaps best known for the discovery of
Herbig–Haro object Herbig–Haro (HH) objects are bright patches of nebula, nebulosity associated with newborn stars. They are formed when narrow jets of partially plasma (physics), ionised gas ejected by stars collide with nearby clouds of gas and dust at several ...
s.


Background

Born in 1920 in Wheeling, West Virginia, Herbig received his
Ph.D A Doctor of Philosophy (PhD, Ph.D., or DPhil; Latin: or ') is the most common Academic degree, degree at the highest academic level awarded following a course of study. PhDs are awarded for programs across the whole breadth of academic fields ...
in 1948 at the
University of California, Berkeley The University of California, Berkeley (UC Berkeley, Berkeley, Cal, or California) is a public land-grant research university in Berkeley, California. Established in 1868 as the University of California, it is the state's first land-grant u ...
; his dissertation is titled ''A Study of
Variable Stars A variable star is a star whose brightness as seen from Earth (its apparent magnitude) changes with time. This variation may be caused by a change in emitted light or by something partly blocking the light, so variable stars are classified as e ...
in Nebulosity''.


Career

His specialty was
star A star is an astronomical object comprising a luminous spheroid of plasma (physics), plasma held together by its gravity. The List of nearest stars and brown dwarfs, nearest star to Earth is the Sun. Many other stars are visible to the naked ...
s at an early stage of
evolution Evolution is change in the heritable characteristics of biological populations over successive generations. These characteristics are the expressions of genes, which are passed on from parent to offspring during reproduction. Variation ...
(a class of intermediate mass pre–main sequence stars are named Herbig Ae/Be stars after him) and the
interstellar medium In astronomy, the interstellar medium is the matter and radiation that exist in the space between the star systems in a galaxy. This matter includes gas in ionic, atomic, and molecular form, as well as dust and cosmic rays. It fills interstella ...
. He was perhaps best known for his discovery, with
Guillermo Haro Guillermo Haro Barraza (; 21 March 1913 – 26 April 1988) was a Mexican astronomer. Through his own astronomical research and the formation of new institutions, Haro was influential in the development of modern observational astronomy in M ...
, of the
Herbig–Haro object Herbig–Haro (HH) objects are bright patches of nebula, nebulosity associated with newborn stars. They are formed when narrow jets of partially plasma (physics), ionised gas ejected by stars collide with nearby clouds of gas and dust at several ...
s; bright patches of nebulosity excited by bipolar outflow from a star being born. Herbig also made prominent contributions to the field of
diffuse interstellar band Diffuse interstellar bands (DIBs) are absorption features seen in the spectra of astronomical objects in the Milky Way and other galaxies. They are caused by the absorption of light by the interstellar medium. Circa 500 bands have now been seen ...
(DIB) research, especially through a series of nine articles published between 1963 and 1995 entitled "The diffuse interstellar bands."


Honors

Awards *
Helen B. Warner Prize for Astronomy The Helen B. Warner Prize for Astronomy is awarded annually by the American Astronomical Society to a young astronomer (aged less than 36, or within 8 years of the award of their PhD) for a significant contribution to observational or theoretical ...
of the
American Astronomical Society The American Astronomical Society (AAS, sometimes spoken as "double-A-S") is an American society of professional astronomers and other interested individuals, headquartered in Washington, DC. The primary objective of the AAS is to promote the adv ...
(1955) *Foreign Scientific Member, Max-Planck-Institut für Astronomie, Heidelberg *
Henry Norris Russell Lectureship The Henry Norris Russell Lectureship is awarded each year by the American Astronomical Society in recognition of a lifetime of excellence in astronomical research. The idea for the lectureship came from then society President Harlow Shapley in 1945, ...
of the AAS (1975) *Médaille, Université de Liège (1969) *
Bruce Medal The Catherine Wolfe Bruce Gold Medal is awarded every year by the Astronomical Society of the Pacific for outstanding lifetime contributions to astronomy. It is named after Catherine Wolfe Bruce, an American patroness of astronomy, and was firs ...
of the Astronomical Society of the Pacific (1980) *Petrie Prize and Lectureship of the
Canadian Astronomical Society The Canadian Astronomical Society (CASCA; french: link=yes, La Société Canadienne d'Astronomie) is a Canadian society of professional astronomers, founded in 1971 and incorporated in 1983. The society is devoted to the promotion and advanceme ...
(1995) Named after him *
Asteroid An asteroid is a minor planet of the inner Solar System. Sizes and shapes of asteroids vary significantly, ranging from 1-meter rocks to a dwarf planet almost 1000 km in diameter; they are rocky, metallic or icy bodies with no atmosphere. ...
11754 Herbig * Herbig Ae/Be stars *
Herbig–Haro object Herbig–Haro (HH) objects are bright patches of nebula, nebulosity associated with newborn stars. They are formed when narrow jets of partially plasma (physics), ionised gas ejected by stars collide with nearby clouds of gas and dust at several ...
s


Selected publications

*"High-Resolution Spectroscopy of
FU Orionis Stars In stellar evolution, an FU Orionis star (also FU Orionis object, or ''FUor'') is a pre–main-sequence star which displays an extreme change in magnitude and spectral type. One example is the star V1057 Cyg, which became 6 magnitudes brighter ...
", ApJ 595 (2003) 384–411 *"The Young Cluster IC 5146", AJ 123 (2002) 304–327 *"Barnard's Merope Nebula Revisited: New Observational Results", AJ 121 (2001) 3138–3148 *"The
Diffuse Interstellar Bands Diffuse interstellar bands (DIBs) are absorption features seen in the spectra of astronomical objects in the Milky Way and other galaxies. They are caused by the absorption of light by the interstellar medium. Circa 500 bands have now been se ...
"
Annu. Rev. Astrophys. 33 (1995) 19–73
*"The Unusual
Pre-Main-Sequence star A pre-main-sequence star (also known as a PMS star and PMS object) is a star in the stage when it has not yet reached the main sequence. Earlier in its life, the object is a protostar that grows by acquiring mass from its surrounding envelope of ...
VY Tauri"
ApJ 360 (1990) 639–649
*"The Structure and Spectrum of R Monocerotis"
ApJ 152 (1968) 439
*"The Spectra of Two Nebulous Objects Near NGC 1999"
ApJ 113 (1951) 697


References


Further reading

* Reipurth, Bo
GEORGE HERBIG and Early Stellar Evolution
Institute for Astronomy, University of Hawaii, Special Publications No. 1. {{DEFAULTSORT:Herbig, George 1920 births Members of the United States National Academy of Sciences American astronomers 2013 deaths University of California, Berkeley alumni University of Hawaiʻi faculty People from Wheeling, West Virginia