
Students Help Astronomers Discover 73 Novae in Andromeda Galaxy
Astronomers, high school teachers and their students have discovered 73 novae in the Andromeda galaxy through a National Science Foundation (NSF) funded education program called "The Use of Astronomy in Research Based Science Education" (RBSE). These results will be presented today by Drs. Travis A. Rector and George H. Jacoby of the National Optical Astronomy Observatory (NOAO), in Tucson, AZ, to the American Astronomical Society meeting in Atlanta, GA. Novae are stellar outbursts that lead to a rapid brightening when mass is transferred between two stars in a binary system, causing the surface layers of one star to ignite explosively from the fusion of hydrogen nuclei. The novae in Andromeda were discovered by students using images from the NSF's Kitt Peak National Observatory and collectively represent the highest discovery rate for novae found in this galaxy. The long-term goal of this project is to accurately determine the novae production rate for galaxies of different sizes and shape, leading to a greater understanding of the frequency of binary stars and distribution of ages of stars in different galaxies. Novae also play a role in creating much of the nitrogen in the universe, an element critical for the creation of life.
Matt Harriger, a student at Harry A. Burke High School, in Omaha, NE, discovered novae in Andromeda through the RBSE program |
For the RBSE novae project, images of galaxies are collected using the NSF's 0.9-meter telescope with a CCD camera on Kitt Peak. Students search images from successive epochs for novae by using a blinking process where images are rapidly alternated using a computer. When a nova appears, its coordinates are recorded. A light curve for each nova is then created by measuring its brightness in each epoch in which it appears. Currently, the RBSE participants are searching for novae in the Andromeda Galaxy, a nearby spiral galaxy similar in stellar content and size to our own Milky Way. A nova is created in a binary star system, where a white dwarf has a nearby companion star. As the companion loses hydrogen gas, the gas falls onto the white dwarf, causing an instability near its surface. An explosive nuclear reaction occurs, causing the white dwarf to shine brightly as a nova.
The NOAO-based RBSE program will hold its fourth annual workshop in Tucson, AZ during the summer of 2000. Additional information, and application materials, can be found at:
http://www.noao.edu/outreach/rbse
NOAO is operated by the Association of Universities for Research in Astronomy, Inc., under cooperative agreement with the National Science Foundation.
For more information:
Suzanne Jacoby
NOAO Education Officer
(520) 318-8364
sjacoby@noao.edu
Dr. Travis A. Rector
Astronomer, NOAO
(520) 318-8256
rector@noao.edu
Tom Gehringer
Teacher, Harry A. Burke High School
tgehring@ops.org
Dr. George Jacoby
Astronomer, NOAO
(520) 318-8292
gjacoby@noao.edu