Gemini: Searching for Orphan Stars Amid Starbirth Fireworks

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Gemini: Searching for Orphan Stars Amid Starbirth Fireworks

Post by bystander » Wed Sep 30, 2015 12:01 am

Searching for Orphan Stars Amid Starbirth Fireworks
Gemini Observatory | 2015 Sep 29
[c][attachment=0]hh24_FINAL[1].jpg[/attachment][/c][hr][/hr]
A new Gemini Observatory image reveals the remarkable “fireworks” that accompany the birth of stars. The image captures in unprecedented clarity the fascinating structures of a gas jet complex emanating from a stellar nursery at supersonic speeds. The striking new image hints at the dynamic (and messy) process of star birth. Researchers believe they have also found a collection of runaway (orphan) stars that result from all this activity..

Gemini Observatory has released one of the most detailed images ever obtained of emerging gas jets streaming from a region of newborn stars. The region, known as the Herbig-Haro 24 (HH 24) Complex, contains no less than six jets streaming from a small cluster of young stars embedded in a molecular cloud in the direction of the constellation of Orion.

"This is the highest concentration of jets known anywhere," says Principal Investigator Bo Reipurth of the University of Hawaii’s Institute for Astronomy (IfA), who adds, "We also think the very dynamic environment causes some of the lowest mass stars in the area to be expelled, and our Gemini data are supporting that idea."

Reipurth along with co-researcher, Colin Aspin, also at the IfA, are using the Gemini North data from the Gemini Multi-Object Spectrograph (GMOS), as well as the Gemini Near-Infrared Imager, to study the region which was discovered in 1963 by George Herbig and Len Kuhi. Located in the Orion B cloud, at a distance of about 400 parsecs, or about 1,300 light-years from our Solar System, this region is rich in young stars and has been extensively studied in all types of light, from radio waves to X-rays.

"The Gemini data are the best ever obtained from the ground of this remarkable jet complex and are showing us striking new detail," says Aspin. Reipurth and Aspin add that they are particularly interested in the fine structure and "excitation distribution" of these jets.

"One jet is highly disturbed, suggesting that the source may be a close binary whose orbit perturbs the jet body," says Reipurth. ...
Attachments
The HH 24 jet complex emanates from a dense cloud core that <br />hosts a small multiple protostellar system known as SSV63. <br />The nebulous star to the south is the visible T Tauri star SSV59. <br />Color image based on the following filters with composite image <br />color assignments in parenthesis: g (blue), r (cyan), I (orange), <br />hydrogen-alpha (red), sulfur II (blue)) images obtained with <br />GMOS on Gemini North in 0.5 arcsecond seeing, and NIRI. <br />Field of view is 4.2x5.1 arcminutes, orientation: north up, <br />east left. Image Credit: Travis Rector.
The HH 24 jet complex emanates from a dense cloud core that
hosts a small multiple protostellar system known as SSV63.
The nebulous star to the south is the visible T Tauri star SSV59.
Color image based on the following filters with composite image
color assignments in parenthesis: g (blue), r (cyan), I (orange),
hydrogen-alpha (red), sulfur II (blue)) images obtained with
GMOS on Gemini North in 0.5 arcsecond seeing, and NIRI.
Field of view is 4.2x5.1 arcminutes, orientation: north up,
east left. Image Credit: Travis Rector.
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