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pro vyhledávání: '"Lee, E'lisa M."'
Autor:
Herczeg, Gregory J., Johnstone, Doug, Mairs, Steve, Hatchell, Jennifer, Lee, Jeong-Eun, Bower, Geoffrey C., Chen, Huei-Ru Vivien, Aikawa, Yuri, Yoo, Hyunju, Kang, Sung-Ju, Kang, Miju, Chen, Wen-Ping, Williams, Jonathan P., Bae, Jaehan, Dunham, Michael M., Vorobiov, Eduard I., Zhu, Zhaohuan, Rao, Ramprasad, Kirk, Helen, Takahashi, Satoko, Morata, Oscar, Lacaille, Kevin, Lane, James, Pon, Andy, Scholz, Aleks, Samal, Manash R., Bell, Graham S., Graves, Sarah, Lee, E'lisa M., Parsons, Harriet, He, Yuxin, Zhou, Jianjun, Kim, Mi-Ryang, Chapman, Scott, Drabek-Maunder, Emily, Chung, Eun Jung, Eyres, Stewart P. S., Forbrich, Jan, Hillenbrand, Lynne A., Inutsuka, Shu-ichiro, Kim, Gwanjeong, Kim, Kyoung Hee, Kuan, Yi-Jehng, Kwon, Woojin, Lai, Shih-Ping, Lalchand, Bhavana, Lee, Chang Won, Lee, Chin-Fei, Long, Feng, Lyo, A-Ran, Qian, Lei, Scicluna, Peter, Soam, Archana, Stamatellos, Dimitris, Takakuwa, Shigehisa, Tang, Ya-Wen, Wang, Hongchi, Wang, Yiren
Most protostars have luminosities that are 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 burs
Externí odkaz:
http://arxiv.org/abs/1709.02052
