Zobrazeno 1 - 10
of 117
pro vyhledávání: '"Bieging, John H."'
Autor:
Bieging, John H., Kong, Shuo
This paper presents maps of the J=2-1 transition of CO toward the Draco Nebula Intermediate Velocity Cloud (IVC). The maps cover 8500 square arcmin with a velocity resolution of 0.33 km~s$^{-1}$ and angular resolution of 38", or 0.11 pc at the cloud
Externí odkaz:
http://arxiv.org/abs/2406.01542
We present CO(2-1) and $^{13}$CO(2-1) maps of the Cygnus-X molecular cloud complex using the 10m Heinrich Hertz Submillimeter Telescope (SMT). The maps cover the southern portion of the complex which is strongly impacted by the feedback from the Cygn
Externí odkaz:
http://arxiv.org/abs/2311.03304
Autor:
Imara, Nia, Lada, Charles, Lewis, John, Bieging, John H., Kong, Shuo, Lombardi, Marco, Alves, Joao
We present a multiwavelength investigation of a region of a nearby giant molecular cloud that is distinguished by a minimal level of star formation activity. With our new (CO)-C-12(J = 2-1) and (CO)-C-13(J = 2-1) observations of a remote region withi
Externí odkaz:
http://hdl.handle.net/10150/624336
http://arizona.openrepository.com/arizona/handle/10150/624336
http://arizona.openrepository.com/arizona/handle/10150/624336
Autor:
Bieging, John H., Patel, Saahil, Peters, William L., Toth, L. Viktor, Marton, Gábor, Zahorecz, Sarolta
We present the results of a program to map the Sh2-235 molecular cloud complex in the CO and (CO)-C-13 J = 2 - 1 transitions using the Heinrich Hertz Submillimeter Telescope. The map resolution is 38 '' (FWHM), with an rms noise of 0.12K brightness t
Externí odkaz:
http://hdl.handle.net/10150/621984
http://arizona.openrepository.com/arizona/handle/10150/621984
http://arizona.openrepository.com/arizona/handle/10150/621984
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:
Bieging, John H., Kong, Shuo
We present maps of 4 galactic giant molecular clouds (GMCs) in the J=2-1 emission of both CO and $^{13}$CO. We use an LTE analysis to derive maps of the CO excitation temperature and column density and the distribution of total molecular gas column d
Externí odkaz:
http://arxiv.org/abs/2209.04535
Autor:
Kohno, Mikito, Omodaka, Toshihiro, Handa, Toshihiro, Chibueze, James O., Nagayama, Takumi, Burns, Ross A., Murase, Takeru, Matsusaka, Ren, Nakano, Makoto, Sunada, Kazuyoshi, Yamada, Rin I., Bieging, John H.
We performed NH$_3\ (J,K)=(1,1),(2,2),$ and $(3,3)$ mapping observations toward the Galactic massive star-forming region Sh 2-255 and Sh 2-257 using the Nobeyama 45-m telescope as a part of the KAGONMA (KAgoshima Galactic Object survey with the Nobey
Externí odkaz:
http://arxiv.org/abs/2202.01518
Autor:
Kang, Miju, Choi, Minho, Wyrowski, Friedrich, Kim, Gwanjeong, Bieging, John H., Kim, Mi-Ryang, Park, Geumsook, Megeath, S. T., Choi, Yunhee, Kang, Sung-Ju, Yoo, Hyunju, Manoj, P.
Ten protostellar outflows in the Orion molecular clouds were mapped in the $^{12}$CO/$^{13}$CO ${J=6\rightarrow5}$ and $^{12}$CO ${J=7\rightarrow6}$ lines. The maps of these mid-$J$ CO lines have an angular resolution of about 10$''$ and a typical fi
Externí odkaz:
http://arxiv.org/abs/2106.07902
Autor:
Yamada, R. I., Sano, H., Tachihara, K., Enokiya, R., Nishimura, A., Fujita, S., Kohno, M., Bieging, John H., Fukui, Y.
W3 is one of the most outstanding regions of high-mass star formation in the outer solar circle, including two active star-forming clouds, W3 Main and W3(OH). Based on a new analysis of the $^{12}$CO data obtained at 38$^{\prime\prime}$ resolution, w
Externí odkaz:
http://arxiv.org/abs/2106.02217
Autor:
Yamada, R. I., Fukui, Y., Sano, H., Tachihara, K., Bieging, John H., Enokiya, R., Nishimura, A., Fujita, S., Kohno, M., Tsuge, Kisetsu
We have carried out a new kinematical analysis of the molecular gas in the Sh2-233 region by using the CO $J$ = 2-1 data taken at $\sim$0.5 pc resolution. The molecular gas consists of a filamentary cloud of 5-pc length with 1.5-pc width where two de
Externí odkaz:
http://arxiv.org/abs/2106.01852