ALMA discovers large 'hot' cocoon around a small baby star

October 4, 2013, National Astronomical Observatory of Japan
Artist impression of a protostar in the Infrared Dark Cloud MM3. The protostar is surrounded by the large hot gas cloud and emanates bipolar gas outflow. Credit: NAOJ

International research team, led by researcher at the University of Electro-Communication observed an infrared dark cloud G34.43+00.24 MM3 with ALMA and discovered a baby star surrounded by a large hot cloud. This hot cloud is about ten times larger than those found around typical solar-mass baby stars. Hot molecular clouds around new-born stars are called "Hot Cores" and have temperature of – 160 degrees Celsius, 100 degrees hotter than normal molecular clouds. The large size of the hot core discovered by ALMA shows that much more energy is emitted from the central baby star than typical solar-mass young stars. This may be due to the higher mass infall rate, or multiplicity of the central baby star. This result indicates a large diversity in the star formation process.

A large hot molecular cloud around a very young star was discovered by ALMA. This hot cloud is about ten times larger than those found around typical solar-mass baby , which indicates that the process has more diversity than ever thought. This result was published in the Astrophysical Journal on September 20th, 2013.

Stars are formed in very cold (-260 degrees Celsius) gas and dust clouds. Infrared Dark Clouds (IRDC) are dense regions of such clouds, and thought that in which clusters of stars are formed. Since most of stars are born as members of star clusters, investigating IRDCs has a crucial role in comprehensive understanding the star formation process.

A baby star is surrounded by the natal gas and dust cloud, and the cloud is warmed up from its center. Temperature of the central part of some, but not all, of such clouds reaches as high as -160 degrees Celsius. Astronomers call those as "hot core" - it may not be hot on the Earth, but is hot enough for a cosmic cloud. Inside hot cores, various molecules, originally trapped in the ice mantle around dust particles, are sublimated. Organic molecules such as methanol (CH3OH), ethyl cyanide (CH3CH2CN), and methyl formate (HCOOCH3) are abundant in hot cores.

Left: Infrared image of the IRDC MM3 taken with NASA MSX satellite. Right: ALMA image of the protostar in MM3 (Red contour: Distribution of methanol molecular emission line, Color image: Distribution of methyl formate molecular line). Credit: UEC/NAOJ

International research team, led by Takeshi Sakai at the University of Electro-Communication, Japan, used ALMA to observe an IRDC named G34.43+00.24 MM3 (hereafter MM3) in the constellation Aquila (the Eagle). They discovered a young object from which the methanol molecular line is strongly emitted. A detailed investigation tells them that the temperature of the methanol gas is -140 degrees Celsius. This shows that MM3 harbors a baby star surrounded by a hot core. The size of the hot core is as large as 800 times 300 astronomical units (au, 1 au equals to the mean distance of the Sun and the Earth; 150 million km). Typical size of hot cores around low-mass young stars is several tens to hundred of au, therefore the hot core in MM3 is exceptionally large. Sakai says "Thanks to the high sensitivity and spatial resolution, we need only a few hours to discover a previously unknown baby star. This is an important step to understand the star formation process in a cluster forming region."

The team also observed radio emission from carbon sulfide (CS) and silicon monoxide (SiO) to reveal the detailed structure of the molecular outflow from the baby star. The speed of the emanated gas is 28 km/s and the extent is 4,400 au. Based on these values, the team calculates the age of the outflow of only 740 years. Although molecular outflows are common features around protostars, the outflow as young as the one in MM3 is quite rare. In summary, ALMA finds that the protostar in MM3 is very young but has a giant hot core.

Why the hot core in MM3 is so large? In order to warm up the large volume of gas, the baby star should emit much more energy than typical ones. Protostars produce emission by converting the gravitational energy of infalling material to the thermal energy. The large size of the hot core in MM3 is possibly due to the high mass infalling rate than ever thought. The other possibility is that two or more protostars are embedded in the hot core. The research team has not reached the reason with this observation yet. "ALMA's spatial resolution improves much more in the near future", Sakai says, "Then much detail of the infalling material toward the protostar can be revealed, and it helps us answer to the mystery behind the diversity in star formation."

Explore further: Hubble eyes a smoldering star

More information: The research findings are presented in the article "ALMA Observations of the IRDC Clump G34.43+00.24 MM3: Hot Core and Molecular Outflows", published in the Astrophysical Journal, Vol. 775, of September 20, 2013.

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1 / 5 (12) Oct 04, 2013
There's that hourglass figure again, strange!
1 / 5 (11) Oct 04, 2013
So why do they know that it is a young star? Because it is surrounded by gas?

Hourglass? Fermi bubbles, anyone?

Group think is dangerous. Look at today's politics.
3 / 5 (6) Oct 04, 2013
There's that hourglass figure again, strange

At negative 160 degrees celcius, it's not plasma. Wake up dude.
1 / 5 (10) Oct 04, 2013
"Temperature" is meaningless as to whether this is plasma, only whether there are free charge carriers present. Even a minutely ionized gas cloud will exhibit the collective effects (EM fields, CIV, et al) of plasmas. The highly organized structure and distribution of the "gas" suggests it has the characteristics of plasma.
5 / 5 (5) Oct 04, 2013
Nothing "strange" about it, that shape is what is expected for a simple jet being slowed by the gas of the nebula, just plain old kinetic energy producing a shock front.

If you want to know the degree of ionisation, look at the spectrum and measure the relative intensities of the various neutral atoms, molecules and ions.

If you want to know if it's a plasma, look at the polarisation.

If you want to believe in EU, don't look at any actual measurements.
5 / 5 (1) Oct 06, 2013
dz^2 orbital ftw!
1.9 / 5 (9) Oct 06, 2013
So why do they know that it is a young star? Because it is surrounded by gas?

Hourglass? Fermi bubbles, anyone?

Group think is dangerous. Look at today's politics.

Idiot, there is no group think, only spectroscopy

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