no code implementations • 11 Mar 2021 • Xunchuan Liu, Y. Wu, C. Zhang, X. Chen, L. -H. Lin, S. -L. Qin, T. Liu, C. Henkel, J. Wang, H. -L. Liu, J. Yuan, L. -X. Yuan, J. Li, Z. -Q. Shen, D. Li, J. Esimbek, K. Wang, L. -X. Li, Kee-Tae Kim, L. Zhu, D. Madones, N. Inostroza, F. -Y. Meng, Tianwei Zhang, K. Tatematsu, Y. Xu, B. -G. Ju, A. Kraus, F. -W. Xu
The signposts of ongoing SCCC and the broadened line widths of C$_3$S and C$_4$H in L1251-1 as well as the distribution of HC$_3$N are also related to outflow activities in this region.
Astrophysics of Galaxies Solar and Stellar Astrophysics
no code implementations • 26 Feb 2021 • N. Falstad, S. Aalto, S. König, K. Onishi, S. Muller, M. Gorski, M. Sato, F. Stanley, F. Combes, E. González-Alfonso, J. G. Mangum, A. S. Evans, L. Barcos-Muñoz, G. C. Privon, S. T. Linden, T. Díaz-Santos, S. Martín, K. Sakamoto, N. Harada, G. A. Fuller, J. S. Gallagher, P. P. van der Werf, S. Viti, T. R. Greve, S. García-Burillo, C. Henkel, M. Imanishi, T. Izumi, Y. Nishimura, C. Ricci, S. Mühle
We find no dependence on the inclination of the host galaxy, but strong evidence of lower IRAS 25 to 60 {\mu}m flux density ratios (f25/f60) in CONs compared to the rest of the sample.
Astrophysics of Galaxies
no code implementations • 22 Dec 2020 • Y. Gong, A. Belloche, F. J. Du, K. M. Menten, C. Henkel, G. X. Li, F. Wyrowski, R. Q. Mao
We performed $^{13}$CO (1--0), C$^{18}$O (1--0), C$^{17}$O (1--0), $^{13}$CO (2--1), C$^{18}$O (2--1), and C$^{17}$O (2--1) imaging observations toward the Serpens filament with the Institut de Radioastronomie Millim{\'e}trique 30-m (IRAM-30 m) and Atacama Pathfinder EXperiment (APEX) telescopes.
Astrophysics of Galaxies
