New research from the Harvard-Smithsonian Center for Astrophysics reveals new insights into how cosmic seeds can grow into massive stars.
Cambridge, Massachusetts – New images from the Smithsonian’s Submillimeter Array (SMA) telescope provide the most detailed view yet of stellar nurseries within the Snake Nebula. These images offer new insights into how cosmic seeds can grow into massive stars.
Stretching across almost 100 light-years of space, the Snake Nebula is located about 11,700 light-years from Earth in the direction of the constellation Ophiuchus. In images from NASA’s Spitzer Space Telescope, it appears as a sinuous, dark tendril against the starry background. It was targeted because it shows the potential to form many massive stars (stars heavier than 8 times our Sun).
“To learn how stars form, we have to catch them in their earliest phases, while they’re still deeply embedded in clouds of gas and dust, and the SMA is an excellent telescope to do so,” explained lead author Ke Wang of the European Southern Observatory (ESO), who started the research as a predoctoral fellow at the Harvard-Smithsonian Center for Astrophysics (CfA).
The team studied two specific spots within the Snake Nebula, designated P1 and P6. Within those two regions, they detected a total of 23 cosmic “seeds” – faintly glowing spots that will eventually birth one or a few stars. The seeds generally weigh between 5 and 25 times the mass of the Sun, and each spans only a few thousand astronomical units (the average Earth-Sun distance). The sensitive, high-resolution SMA images not only unveil the small seeds, but also differentiate them in age.
Previous theories proposed that high-mass stars form within very massive, isolated “cores” weighing at least 100 times the mass of the Sun. These new results show that that is not the case. The data also demonstrate that massive stars aren’t born alone but in groups.
“High-mass stars form in villages,” said co-author Qizhou Zhang of the CfA. “It’s a family affair.”
The team also was surprised to find that these two nebular patches had fragmented into individual star seeds so early in the star formation process.
They detected bipolar outflows and other signs of active, ongoing star formation. Eventually, the Snake Nebula will dissolve and shine as a chain of several star clusters.
These results are published in the Monthly Notices of the Royal Astronomical Society.
Headquartered in Cambridge, Massachusetts, the Harvard-Smithsonian Center for Astrophysics (CfA) is a joint collaboration between the Smithsonian Astrophysical Observatory and the Harvard College Observatory. CfA scientists, organized into six research divisions, study the origin, evolution and ultimate fate of the universe.
Reference: “Hierarchical fragmentation and differential star formation in the Galactic ‘Snake’: infrared dark cloud G11.11−0.12” by Ke Wang, Qizhou Zhang, Leonardo Testi, Floris van der Tak, Yuefang Wu, Huawei Zhang, Thushara Pillai, Friedrich Wyrowski, Sean Carey, Sarah E. Ragan and Thomas Henning, 24 February 2014, MNRAS.
DOI: 10.1093/mnras/stu127
arXiv:1401.4157
Never miss a breakthrough: Join the SciTechDaily newsletter.
Follow us on Google and Google News.