Add to ORKGMost protostars have luminosities that are significantly fainter than expected from steady accretion over the protostellar lifetime.The solution to this problem may lie in episodic mass accretion--prolonged periods of very low accretion punctuated by short bursts of rapid accretion.Most protostars have luminosities that are significantly fainter than expected from steady accretion over the protostellar lifetime.The solution to this problem may lie in episodic mass accretion--prolonged periods of very low accretion punctuated by short bursts of rapid accretion.中国天文学会
It is speculated that the accretion of material onto young protostars is episodic. We present a comp...
The formation and evolution of protoplanetary disks are fundamental in the process of low-mass star ...
During the protostellar phase of stellar evolution, accretion is expected to be variable, but this v...
textA long-standing problem in low-mass star formation is the "luminosity problem," whereby protosta...
Most protostars have luminosities that are fainter than expected from steady accretion over the prot...
A star acquires much of its mass by accreting material from a disk. Accretion is probably not contin...
textA wide range of observed luminosities of young forming stars conflicts with predictions of the s...
This is an author-created, uncopyedited version of an article published in The Astrophysical Journal...
This is the final version. Available from American Astronomical Society via the DOI in this recordMo...
One of the outstanding open questions in the star formation is, when does the star attain most of it...
A long-standing problem in low-mass star formation is the "luminosity problem," whereby protostars a...
Context. Understanding how protostars accrete their mass is a central question of star for...
Following our recent work devoted to the effect of accretion on the pre-main-sequence evolution of l...
Accretion through circumstellar disks plays an important role in star formation and in establishing ...
A fundamental question in astrophysics is how stars get their mass. We know that low-mass stars form...
It is speculated that the accretion of material onto young protostars is episodic. We present a comp...
The formation and evolution of protoplanetary disks are fundamental in the process of low-mass star ...
During the protostellar phase of stellar evolution, accretion is expected to be variable, but this v...
textA long-standing problem in low-mass star formation is the "luminosity problem," whereby protosta...
Most protostars have luminosities that are fainter than expected from steady accretion over the prot...
A star acquires much of its mass by accreting material from a disk. Accretion is probably not contin...
textA wide range of observed luminosities of young forming stars conflicts with predictions of the s...
This is an author-created, uncopyedited version of an article published in The Astrophysical Journal...
This is the final version. Available from American Astronomical Society via the DOI in this recordMo...
One of the outstanding open questions in the star formation is, when does the star attain most of it...
A long-standing problem in low-mass star formation is the "luminosity problem," whereby protostars a...
Context. Understanding how protostars accrete their mass is a central question of star for...
Following our recent work devoted to the effect of accretion on the pre-main-sequence evolution of l...
Accretion through circumstellar disks plays an important role in star formation and in establishing ...
A fundamental question in astrophysics is how stars get their mass. We know that low-mass stars form...
It is speculated that the accretion of material onto young protostars is episodic. We present a comp...
The formation and evolution of protoplanetary disks are fundamental in the process of low-mass star ...
During the protostellar phase of stellar evolution, accretion is expected to be variable, but this v...