A team of astronomers led by Prof. HAN Zhanwen from the Yunnan Observatories
(YAO) of the Chinese Academy of Sciences and Prof. Chris Wolf from
Australian National University has jointly discovered a binary system
ejecting a common envelope at a speed of about 200 kilometers per second.
This is the first time scientists have observed direct evidence of common
envelope evolution, which is a key process of binary star evolution. This
important discovery provides a way to accurately characterize the common
envelope evolution of binary stars through observation.
The study was published in Monthly Notices of the Royal Astronomical Society
on July 7.
Most of the luminous objects in the Universe are stars. More than half of
all stars are found to be in binary systems. Two stars in a binary system
orbit around each other due to their gravitational attraction.
Binary evolution plays an important role in determining the fate of stellar
objects. It has been widely used as the explanation for most mysteries in
astronomy and astrophysics such as the formation of exotic stellar objects
including Type Ia supernovae, double black holes, and double neutron stars,
etc.
Common envelope evolution is one of the key processes of binary evolution.
In this process, the donor star of a binary system expands dramatically due
to the mass loss, thus leading to the two stars spiraling towards each other
and formation of a common envelope. This process determines the subsequent
evolution of the binary system. A binary system with a shorter orbital
period would be expected to form if the common envelope is ejected
successfully. Otherwise, the two stars within the common envelope would
merge into a single object.
Common envelopes were first postulated by B. Paczynski in 1976. However, a
common envelope had never been seen before now. As a consequence, scientists
were quite unclear what exactly happens during the common envelope phase of
binary star evolution.
Based on the observations from the Australian National University's
2.3-meter wide-field telescope and the Kepler telescope, Chinese and
Australian scientists have jointly found a binary system consisting of a hot
subdwarf and a white dwarf, named J 1920. In this binary system, the two
stars orbit around each other with an orbital period of about 3.5 hours, and
are getting closer and closer.
In addition, scientists have seen that this binary system is surrounded by
an expanding shell moving at a speed of about 200 kilometers per second.
This expanding shell is further confirmed to be a common envelope that was
ejected from the binary system about 10,000 years ago. Continuous orbital
contraction observed in the J 1920 binary system indicates that friction
caused by the orbital motion of the two stars in the envelope can severely
dissipate orbital angular momentum. This is a new mechanism for angular
momentum loss in addition to the mechanisms of magnetic breaking and
gravitational radiation.
The significance of this important discovery is that it turns a theoretical
idea into reality. Scientists have not only seen the first evidence of
common envelope evolution, but have also been able to accurately
characterize the common envelope evolution of binary stars through
observation.
Reference:
Jiangdan Li, Christopher A Onken et. al, “A Roche Lobe-filling hot
Subdwarf and White Dwarf Binary: Possible detection of an ejected common
envelope?”, Monthly Notices of the Royal Astronomical Society.
DOI: 10.1093/mnras/stac1768
Tags:
Space & Astrophysics