FACTOID # 124: Teachers make up 7.8 percent of Iceland’s labor force - and they only have to teach 38 weeks per year.
 
 Home   Encyclopedia   Statistics   Countries A-Z   Flags   Maps   Education   Forum   FAQ   About 
 
 
 
WHAT'S NEW
RECENT ARTICLES
More Recent Articles »
 

SEARCH ALL

FACTS & STATISTICS    Advanced view

Search encyclopedia, statistics and forums:

 

 

(* = Graphable)

 

 


Encyclopedia > Dr. Guillermo Haro

1913-1988


Profesor Haro was born in Mexico City on March 21st, 1913. He grew up in the same city and studied Philosophy at the University of Mexico. He became interested in astronomy and because of his dedication and enthusiasm was hired in 1943 as an assistant at the newly founded Observatorio Astrofísica de Tonantzintla. In order to pursue his astronomical training he visited the US and worked from 1943 to 1944 at Harvard College Observatory.


Upon his return to Mexico in 1945 he continued working at the Observatorio Astrofísico de Tonantzintla where he was responsible for the commissioning of the new 24-31 inch Schmidt camera and where he became involved in the study of extremely red and extremely blue stars. In 1947 he started working for the Observatorio de Tacubaya of the Universidad Nacional Autónoma de México.


Guillermo Haro make many contributions to observational astronomy, especially with the Tonantzintla Schmidt telescope. Among them were the detection of a large number of planetary nebulae in the direction of the galactic center and the discovery (also independently done by G. Herbig) of the nonstellar condensations in high density clouds near regions of recent star formation, now called Herbig-Haro objects. Haro and co-workers discovered flare stars in the Orion nebula region, and later on in stellar aggregates of different ages. His intense activity detecting flare stars continued till the end of his life.


Other major research projects carried out by Haro included the list of 8746 blue stars in the direction of the North Galactic Pole published jointly with W. J. Luyten in 1961, work made with the 48 inch Palomar Schmidt using the three-color image technique developed at Tonantzintla. At least 50 of these objects turned out to be quasars (which had not yet been discovered in 1961). Haro’s list of 44 blue galaxies, compiled in 1956, was a precursor to the work of Markarian and others in searching for such galaxies. Haro also discovered a number of T Tauri Stars, one supernova, more than 10 novae and one comet.


Guillermo Haro was very influential in the development of astronomy in Mexico, not only by carrying out his own astronomical research, and promoting the development of new institutions, but in a more important aspect, by defining modern astrophysical research in Mexico where he gave impulse to different initial lines of research and established general scientific policies.



 
 

COMMENTARY     


Share your thoughts, questions and commentary here
Your name
Your comments

Want to know more?
Search encyclopedia, statistics and forums:

 


Lesson Plans | Student Area | Student FAQ | Reviews | Press Releases |  Feeds | Contact
The Wikipedia article included on this page is licensed under the GFDL.
Images may be subject to relevant owners' copyright.
All other elements are (c) copyright NationMaster.com 2003-5. All Rights Reserved.
Usage implies agreement with terms, 1022, m