[Right] A NASA Hubble Telescope (HST) image of NGC 1741, a pair of colliding galaxies are undergoing a burst star formation as a result of a collision.
The results from this observations are being presented to the American Astronomical Society meeting in Berkeley, California.
The Hubble pictures illustrates dramatic new details of the starburst phenomena that result from the merger between to galaxies. NGC 1741 contains a pair of starburst centers that are separated by 3,000 light-years (4 arc seconds at the galaxy's distance of 50 Megaparsecs). The HST image resolves several very young and compact starburst regions about 150 to 300 light-years across, which are embedded in double-lobed structure. Each contains several hundred to a thousand recently formed massive stars. HST reveals for the first time more luminous (and contain several times as many hot stars) as 30 Doradus, a nearby prototype starburst in the Large Magellanic Cloud.
Previous ground-based spectroscopic studies show that the most massive stars are less than ten million years old, and burst of massive stars such as these have occurred only for a million years or less. The HST UV picture was taken using the European Space Agency's Faint Object Camera (FOC).
The investigators hope to obtain HST spectra of the individual starburst knots in NGC 1741 once HST's optics are improved during a Space Shuttle servicing mission scheduled for late 1993. The spectra will allow astronomers to more accurately estimate the ages of the hot stars in each clump. This would show whether the individual starburst knots have formed simultaneously or sequentially.
[Left] A ground based telescopic image of galaxy NGC 1741 is located 150 million light-years away in the constellation Eridamus. The galaxy's peculiar shape and double-lobed structure is evidence for a recent merger between two galaxies.
Credits
Right: Dr. Peter Conti (University or Colorado) /NASA & ESA; Co-investigators [alphbetical]: Alex Filippenko, UC Berkeley; Claus Leither, STScI; Carmelle Robert, STScI; Wal Sargent, CalTech; and William Vacca, UC Berkeley.;Left: Todd Small (Cal Tech)
| About The Object | |
|---|---|
| Object Name | NGC 1741 |
| R.A. Position | 05h 1m 38.29s |
| Dec. Position | -4° 15' 24.99" |
| About The Object | |
|---|---|
| Object Name | A name or catalog number that astronomers use to identify an astronomical object. |
| Object Description | The type of astronomical object. |
| R.A. Position | Right ascension – analogous to longitude – is one component of an object's position. |
| Dec. Position | Declination – analogous to latitude – is one component of an object's position. |
| Constellation | One of 88 recognized regions of the celestial sphere in which the object appears. |
| Distance | The physical distance from Earth to the astronomical object. Distances within our solar system are usually measured in Astronomical Units (AU). Distances between stars are usually measured in light-years. Interstellar distances can also be measured in parsecs. |
| Dimensions | The physical size of the object or the apparent angle it subtends on the sky. |
| About The Data | |
| Data Description |
|
| Instrument | The science instrument used to produce the data. |
| Exposure Dates | The date(s) that the telescope made its observations and the total exposure time. |
| Filters | The camera filters that were used in the science observations. |
| About The Image | |
| Image Credit | The primary individuals and institutions responsible for the content. |
| Publication Date | The date and time the release content became public. |
| Color Info | A brief description of the methods used to convert telescope data into the color image being presented. |
| Orientation | The rotation of the image on the sky with respect to the north pole of the celestial sphere. |
