Zobrazeno 1 - 10
of 5 783
pro vyhledávání: '"A, Pelkonen"'
Protoplanetary disks are routinely described as finite mass reservoirs left over by the gravitational collapse of the protostar, an assumption that strongly constrains both disk evolution and planet formation models. We propose a different scenario w
Externí odkaz:
http://arxiv.org/abs/2405.07334
Context. While Class II stars have already accreted most of their mass, the continued inflow of fresh material via Bondi-Hoyle accretion acts as an additional mass reservoir for their circumstellar disks. This may explain the observed accretion rates
Externí odkaz:
http://arxiv.org/abs/2405.06520
Autor:
Zhu, Zhi-Kai, Fang, Min, Lu, Zu-Jia, Wang, Junzhi, Li, Guang-Xing, Zhang, Shiyu, Pelkonen, Veli-Matti, Padoan, Paolo, Liang, En-Wei
The kinematic information of the Radcliffe Wave (RW) is essential for determining its existence and gaining insights into its origin and evolution. In this work, we present an accurate measurement of the vertical velocity ($V_Z$) of RW by incorporati
Externí odkaz:
http://arxiv.org/abs/2402.15346
The ages of young star clusters are fundamental clocks to constrain the formation and evolution of pre-main-sequence stars and their protoplanetary disks and exoplanets. However, dating methods for very young clusters often disagree, casting doubts o
Externí odkaz:
http://arxiv.org/abs/2311.08363
Autor:
Anna-Maria Pelkonen, Päivi Rajavaara, Hannu Vähänikkilä, Vuokko Anttonen, Marja-Liisa Laitala
Publikováno v:
BMC Oral Health, Vol 24, Iss 1, Pp 1-7 (2024)
Abstract Background Determining risk indicators behind dental caries is important for identifying children in need of enhanced dental care. The aim of this register-based study was to investigate the association of family-related risk indicators and
Externí odkaz:
https://doaj.org/article/e0b2cb4ea3df4fe5b824db96c23d4c37
Characterizing prestellar cores in star-forming regions is an important step towards the validation of theoretical models of star formation. Thanks to their sub-arcsecond resolution, ALMA observations can potentially provide samples of prestellar cor
Externí odkaz:
http://arxiv.org/abs/2301.07398
Autor:
Tiina Helena Tanninen, MD, Anna Susanna Pelkonen, MD, PhD, Leo Pekka Malmberg, MD, PhD, Mika Juhani Mäkelä, MD, PhD
Publikováno v:
Journal of Allergy and Clinical Immunology: Global, Vol 3, Iss 3, Pp 100268- (2024)
Background: The combination of an inhaled corticosteroid (ICS) and long-acting β-agonist (LABA) (ICS/LABA) has shown superiority in improving lung function (FEV1) compared with an ICS alone. The clinical effect of a ICS/LABA combination depends on t
Externí odkaz:
https://doaj.org/article/25294ea070cb4c788150820276edc60c
Autor:
Dutta, Somnath, Lee, Chin-Fei, Hirano, Naomi, Liu, Tie, Johnstone, Doug, Liu, Sheng-Yuan, Tatematsu, Kenichi, Goldsmith, Paul F., Sahu, Dipen, Evans, Neal J., Sanhueza, Patricio, Kwon, Woojin, Qin, Sheng-Li, Samal, Manash Ranjan, Zhang, Qizhou, Kim, Kee-Tae, Shang, Hsien, Lee, Chang Won, Moraghan, Anthony, Jhan, Kai-Syun, Li, Shanghuo, Lee, Jeong-Eun, Traficante, Alessio, Juvela, Mika, Bronfman, Leonardo, Eden, David, Soam, Archana, He, Jinhua, Liu, Hong-li, Kuan, Yi-Jehng, Pelkonen, Veli-Matti, Luo, Qiuyi, Yi, Hee-Weon, Hsu, Shih-Ying
Protostellar outflows and jets play a vital role in star formation as they carry away excess angular momentum from the inner disk surface, allowing the material to be transferred toward the central protostar. Theoretically, low velocity and poorly co
Externí odkaz:
http://arxiv.org/abs/2204.06661
Autor:
Luo, Qiuyi, Liu, Tie, Tatematsu, Kenichi, Liu, ShengYuan, Li, Pak Shing, di Francesco, James, Johnstone, Doug, Goldsmith, Paul F., Dutta, Somnath, Hirano, Naomi, Lee, ChinFei, Li, Di, Kim, KeeTae, Lee, Chang Won, Lee, JeongEun, Liu, Xunchuan, Juvela, Mika, He, Jinhua, Qin, ShengLi, Liu, HongLi, Eden, David, Kwon, Woojin, Sahu, Dipen, Li, Shanghuo, Xu, FengWei, Zhang, Siju, Hsu, ShihYing, Bronfman, Leonardo, Sanhueza, Patricio, Pelkonen, VeliMatti, Zhou, Jianwen, Liu, Rong, Gu, Qilao, Wu, Yuefang, Mai, Xiaofeng, Falgarone, Edith, Shen, ZhiQiang
During the transition phase from a prestellar to a protostellar cloud core, one or several protostars can form within a single gas core. The detailed physical processes of this transition, however, still remain unclear. We present 1.3 mm dust continu
Externí odkaz:
http://arxiv.org/abs/2204.06176
Publikováno v:
In Journal of Environmental Chemical Engineering October 2024 12(5)