Zobrazeno 1 - 10
of 48
pro vyhledávání: '"Kim, Jinyoung S."'
Autor:
Haworth, Thomas J., Reiter, Megan, O'Dell, C. Robert, Zeidler, Peter, Berne, Olivier, Manara, Carlo F., Ballabio, Giulia, Kim, Jinyoung S., Bally, John, Goicoechea, Javier R., Aru, Mari-Liis, Gupta, Aashish, Miotello, Anna
We present VLT/MUSE Narrow Field Mode (NFM) observations of a pair of disc-bearing young stellar objects towards the Orion Bar: 203-504 and 203-506. Both of these discs are subject to external photoevaporation, where winds are launched from their out
Externí odkaz:
http://arxiv.org/abs/2308.12342
Autor:
Da Rio, Nicola, Tan, Jonathan C., Covey, Kevin R., Cottaar, Michiel, Foster, Jonathan B., Cullen, Nicholas C., Tobin, John, Kim, Jinyoung S., Meyer, Michael R., Nidever, David L., Stassun, Keivan G., Chojnowski, S. Drew, Flaherty, Kevin M., Majewski, Steven R., Skrutskie, Michael F., Zasowski, Gail, Pan, Kaike
The kinematics and dynamics of young stellar populations enable us to test theories of star formation. With this aim, we continue our analysis of the SDSS-III/APOGEE IN-SYNC survey, a high-resolution near-infrared spectroscopic survey of young cluste
Externí odkaz:
http://hdl.handle.net/10150/625776
http://arizona.openrepository.com/arizona/handle/10150/625776
http://arizona.openrepository.com/arizona/handle/10150/625776
Autor:
Lim, Beomdu, Sung, Hwankyung, Kim, Jinyoung S., Bessell, Michael S., Hwang, Narae, Park, Byeong-Gon
The timescale of cluster formation is an essential parameter in order to understand the formation process of star clusters. Pre-main sequence (PMS) stars in nearby young open clusters reveal a large spread in brightness. If the spread were considered
Externí odkaz:
http://hdl.handle.net/10150/622162
http://arizona.openrepository.com/arizona/handle/10150/622162
http://arizona.openrepository.com/arizona/handle/10150/622162
Autor:
Jose, Jessy, Kim, Jinyoung S., Herczeg, Gregory J., Samal, Manash R., Bieging, John H., Meyer, Michael R., Sherry, William H.
One of the key questions in the field of star formation is the role of stellar feedback on the subsequent star formation process. The W3 giant molecular cloud complex at the western border of the W4 super bubble is thought to be influenced by the mas
Externí odkaz:
http://hdl.handle.net/10150/621216
http://arizona.openrepository.com/arizona/handle/10150/621216
http://arizona.openrepository.com/arizona/handle/10150/621216
Autor:
Haworth, Thomas J., Kim, Jinyoung S., Qiao, Lin, Winter, Andrew J., Williams, Jonathan P., Clarke, Cathie J., Owen, James E., Facchini, Stefano, Ansdell, Megan, Kama, Mikhel, Ballabio, Giulia
We used the Atacama Pathfinder Experiment (APEX) telescope to search for CI 1-0 (492.16GHz) emission towards 8 proplyds in NGC 1977, which is an FUV radiation environment two orders of magnitude weaker than that irradiating the Orion Nebular Cluster
Externí odkaz:
http://arxiv.org/abs/2203.03928
Young open clusters are ideal laboratories to understand star formation process. We present deep UBV I and Halpha photometry for the young open cluster IC 1590 in the center of the H II region NGC 281. Early-type members are selected from UBV photome
Externí odkaz:
http://arxiv.org/abs/2106.15129
Autor:
Haworth, Thomas J., Kim, Jinyoung S., Winter, Andrew J., Hines, Dean C., Clarke, Cathie J., Sellek, Andrew D., Ballabio, Giulia, Stapelfeldt, Karl R.
A recent survey of the inner $0.35\times0.35$pc of the NGC 2024 star forming region revealed two distinct millimetre continuum disc populations that appear to be spatially segregated by the boundary of a dense cloud. The eastern (and more embedded) p
Externí odkaz:
http://arxiv.org/abs/2012.09166
Autor:
Lim, Beomdu, Hong, Jongsuk, Yun, Hyeong-Sik, Hwang, Narae, Kim, Jinyoung S., Lee, Jeong-Eun, Park, Byeong-Gon, Park, Sunkyung
Stellar kinematics provides the key to understanding the formation process and dynamical evolution of stellar systems. Here, we present a kinematic study of the massive star-forming region W4 in the Cassiopeia OB6 association using the Gaia Data Rele
Externí odkaz:
http://arxiv.org/abs/2006.15262
Autor:
Jose, Jessy, Kim, Jinyoung S., Herczeg, Gregory J., Samal, Manash R., Bieging, John H., Meyer, Michael R., Sherry, William H.
One of the key questions in the field of star formation is the role of stellar feedback on subsequent star formation process. The W3 giant molecular cloud complex at the western border of the W4 super bubble is thought to be influenced by the stellar
Externí odkaz:
http://arxiv.org/abs/1602.06212
Autor:
Da Rio, Nicola, Tan, Jonathan C., Covey, Kevin R., Cottaar, Michiel, Foster, Jonathan B., Cullen, Nicholas C., Tobin, John J., Kim, Jinyoung S., Meyer, Michael R., Nidever, David L., Stassun, Keivan G., Chojnowski, S. Drew, Flaherty, Kevin M., Majewski, Steve, Skrutskie, Michael F., Zasowski, Gail, Pan, Kaike
We present the results of the SDSS APOGEE INfrared Spectroscopy of Young Nebulous Clusters program (IN-SYNC) survey of the Orion A molecular cloud. This survey obtained high resolution near infrared (NIR) spectroscopy of about 2700 young pre-main seq
Externí odkaz:
http://arxiv.org/abs/1511.04147