Zobrazeno 1 - 10
of 97
pro vyhledávání: '"Wright, M. C. H."'
Autor:
Chen, Huei-Ru Vivien, Zhang, Qizhou, Wright, M. C. H., Busquet, Gemma, Lin, Yuxin, Liu, Hauyu Baobab, Olguin, F. A., Sanhueza, Patricio, Nakamura, Fumitaka, Palau, Aina, Ohashi, Satoshi, Tatematsu, Ken'ichi, Liao, Li-Wen
Filaments are ubiquitous structures in molecular clouds and play an important role in the mass assembly of stars. We present results of dynamical stability analyses for filaments in the infrared dark cloud G14.225$-$0.506, where a delayed onset of ma
Externí odkaz:
http://arxiv.org/abs/1903.04376
Autor:
Wright, M. C. H., Plambeck, R. L.
We present ALMA images of the dust and molecular line emission in the Orion Hot Core at 349 GHz. At 0.2" angular resolution the images reveal multiple clumps in an arc ~ 1" east of Orion Source I, the protostar at the center of the Kleinmann-Low Nebu
Externí odkaz:
http://arxiv.org/abs/1705.03957
Autor:
Plambeck, R. L., Wright, M. C. H.
Orion Source I (`SrcI') is the protostar at the center of the Kleinmann-Low Nebula. ALMA observations of SrcI with 0.2" angular resolution were made at 350 and 660 GHz to search for the H26alpha and H21alpha hydrogen recombination lines and to measur
Externí odkaz:
http://arxiv.org/abs/1608.00996
We present dust polarization and CO molecular line images of NGC 7538 IRS1. We combined data from the SMA, CARMA and JCMT telescopes to make images with 2.5 arcsec resolution at 230 and 345 GHz. The images show a remarkable spiral pattern in both the
Externí odkaz:
http://arxiv.org/abs/1410.2269
Autor:
Plambeck, R. L., Bolatto, A. D., Carpenter, J. M., Eisner, J. A., Lamb, J. W., Leitch, E. M., Marrone, D. P., Muchovej, S. J., Perez, L. M., Pound, M. W., Teuben, P. J., Volgenau, N. H., Woody, D. P., Wright, M. C. H., Zauderer, B. A.
The 229 GHz (lambda 1.3mm) radio emission from Orion-KL was mapped with up to 0.14" angular resolution with CARMA, allowing measurements of the flux densities of Source I ('SrcI') and the Becklin-Neugebauer Object (BN), the 2 most massive stars in th
Externí odkaz:
http://arxiv.org/abs/1211.0085
Autor:
ATA GROUP, Atkinson, Shannon, Backer, D. C., Backus, P. R., Barott, William, Bauermeister, Amber, Blitz, Leo, Bock, D. C. -J., Bower, Geoffrey C., Bradford, Tucker, Cheng, Calvin, Croft, Steve, Dexter, Matt, Dreher, John, Engargiola, Greg, Fields, Ed, Heiles, Carl, Helfer, Tamara, Jordan, Jane, Jorgensen, Susan, Kilsdonk, Tom, Gutierrez-Kraybill, Colby, Keating, Garrett, Law, Casey, Lugten, John, MacMahon, D. H. E., McMahon, Peter, Milgrome, Oren, Siemion, Andrew, Smolek, Ken, Thornton, Douglas, Pierson, Tom, Randall, Karen, Ross, John, Shostak, Seth, Tarter, J. C., Urry, Lynn, Werthimer, Dan, Williams, Peter K. G., Whysong, David, Harp, G. R., Ackermann, R. F., Nadler, Z. J., Blair, Samantha K., Davis, M. M., Wright, M. C. H., Forster, J. R., DeBoer, D. R., Welch, W. J.
Publikováno v:
IEEE Transactions on Antennas and Propagation, 59 (2011) p. 2004
The Allen Telescope Array (ATA) is a cm-wave interferometer in California, comprising 42 antenna elements with 6-m diameter dishes. We characterize the antenna optical accuracy using two-antenna interferometry and radio holography. The distortion of
Externí odkaz:
http://arxiv.org/abs/1210.8246
Autor:
Zhao, Jun-Hui, Wright, M. C. H.
The ionized core in the Sgr B2 Main star-forming region was imaged using the Submillimeter Array archival data observed for the H26$\alpha$ line and continuum emission at 0.86 millimeter with an angular resolution 0.3\arcsec. Eight hyper-compact H26$
Externí odkaz:
http://arxiv.org/abs/1108.0916
We report new results on outflow and infall in the star forming cores W3-SE SMA-1 and SMA-2 based on analysis of $\sim2.5\arcsec$ resolution observations of the molecular lines HCN(3-2), HCO$^+$(3-2), N$_2$H$^+$(3-2) and CH$_3$OH(5$_{2,3}-4_{1,3}$) w
Externí odkaz:
http://arxiv.org/abs/1108.0713
Autor:
Enoch, M. L., Corder, S., Duchene, G., Bock, D. C., Bolatto, A. D., Culverhouse, T. L., Kwon, W., Lamb, J. W., Leitch, E. M., Marrone, D. P., Muchovej, S. J., Perez, L. M., Scott, S. L., Teuben, P. J., Wright, M. C. H., Zauderer, B. A.
We present high-resolution CARMA 230 GHz continuum imaging of nine deeply embedded protostars in the Serpens Molecular Cloud, including six of the nine known Class 0 protostars in Serpens. This work is part of a program to characterize disk and envel
Externí odkaz:
http://arxiv.org/abs/1106.1899
Autor:
Koda, J., Sawada, T., Wright, M. C. H., Teuben, P., Corder, S. A., Patience, J., Scoville, N., Meyer, J. Donovan, Egusa, F.
We report the CO(J=1-0) observations of M51 using both the Combined Array for Research in Millimeter Astronomy (CARMA) and the Nobeyama 45m telescope (NRO45). We describe a procedure for the combination of interferometer and single-dish data. In part
Externí odkaz:
http://arxiv.org/abs/1102.3060