Zobrazeno 1 - 10
of 208
pro vyhledávání: '"Cunningham M. R."'
Publikováno v:
Open Astronomy, Vol 20, Iss 4, Pp 558-565 (2011)
Although hydrogen cyanide has become quite a common molecular tracing species for a variety of astrophysical sources, it, however, exhibits dramatic non-LTE behaviour in its hyperfine line structure. Individual hyperfine components can be strongly bo
Externí odkaz:
https://doaj.org/article/4428f4a56d184ceaa1b8c0acf8b7200c
Autor:
Dawson, J. R., Jones, P. A., Purcell, C., Walsh, A. J., Breen, S. L., Brown, C., Carretti, E., Cunningham, M. R., Dickey, J. M., Ellingsen, S. P., Gibson, S. J., Gomez, J. F., Green, J. A., Imai, H., Krishnan, V., Lo, N., Lowe, V., Marquarding, M., McClure-Griffiths, N. M.
We present the full data release for the Southern Parkes Large-Area Survey in Hydroxyl (SPLASH), a sensitive, unbiased single-dish survey of the Southern Galactic Plane in all four ground-state transitions of the OH radical at 1612, 1665, 1667 and 17
Externí odkaz:
http://arxiv.org/abs/2203.05131
Autor:
Denes, H., Jones, P. A., Toth, L. V., Zahorecz, S., Koo, B-C., Pinter, S., Racz, I. I., Balazs, L. G., Cunningham, M. R., Doi, Y., Horvath, I., Kovacs, T., Onishi, T., Suleiman, N., Bagoly, Z.
The afterglow of a gamma ray burst (GRB) can give us valuable insight into the properties of its host galaxy. To correctly interpret the spectra of the afterglow we need to have a good understanding of the foreground interstellar medium (ISM) in our
Externí odkaz:
http://arxiv.org/abs/1909.00622
Probing magnetic fields in Giant Molecular Clouds is often challenging. Fortunately, recently simulations show that analysis of velocity gradients (the Velocity Gradient Technique) can be used to map out the magnetic field morphology of different phy
Externí odkaz:
http://arxiv.org/abs/1904.04391
Autor:
Eden, D. J., Liu, Tie, Kim, Kee-Tae, Liu, S. -Y., Tatematsu, K., Di Francesco, J., Wang, K., Wu, Y., Thompson, M. A., Fuller, G. A., Li, Di, Ristorcelli, I., Kang, Sung-ju, Hirano, N., Johnstone, D., Lin, Y., He, J. H., Koch, P. M., Sanhueza, Patricio, Qin, S. -L., Zhang, Q., Goldsmith, P. F., Evans II, N. J., Yuan, J., Zhang, C. -P., White, G. J., Choi, Minho, Lee, Chang Won, Toth, L. V., Mairs, S., Yi, H. -W., Tang, M., Soam, A., Peretto, N., Samal, M. R., Fich, M., Parsons, H., Malinen, J., Bendo, G. J., Rivera-Ingraham, A., Liu, H. -L., Wouterloot, J., Li, P. S., Qian, L., Rawlings, J., Rawlings, M. G., Feng, S., Wang, B., Li, Dalei, Liu, M., Luo, G., Marston, A. P., Pattle, K. M., Pelkonen, V. -M., Rigby, A. J., Zahorecz, S., Zhang, G., Bogner, R., Aikawa, Y., Akhter, S., Alina, D., Bell, G., Bernard, J. -P., Blain, A., Bronfman, L., Byun, D. -Y., Chapman, S., Chen, H. -R., Chen, M., Chen, W. -P., Chen, X., Chen, Xuepeng, Chrysostomou, A., Chu, Y. -H., Chung, E. J., Cornu, D., Cosentino, G., Cunningham, M. R., Demyk, K., Drabek-Maunder, E., Doi, Y., Eswaraiah, C., Falgarone, E., Feher, O., Fraser, H., Friberg, P., Garay, G., Ge, J. X., Gear, W. K., Greaves, J., Guan, X., Harvey-Smith, L., Hasegawa, T., He, Y., Henkel, C., Hirota, T., Holland, W., Hughes, A., Jarken, E., Ji, T. -G., Jimenez-Serra, I., Kang, Miju, Kawabata, K. S., Kim, Gwanjeong, Kim, Jungha, Kim, Jongsoo, Kim, S., Koo, B. -C., Kwon, Woojin, Kuan, Y. -J., Lacaille, K. M., Lai, S. -P., Lee, C. F., Lee, J. E., Lee, Y. -U., Li, H., Lo, N., Lopez, J. A. P., Lu, X., Lyo, A. -R., Mardones, D., McGehee, P., Meng, F., Montier, L., Montillaud, J., Moore, T. J. T., Morata, O., Moriarty-Schieven, G. H., Ohashi, S., Pak, S., Park, Geumsook, Paladini, R., Pech, G., Qiu, K., Ren, Z. -Y., Richer, J., Sakai, T., Shang, H., Shinnaga, H., Stamatellos, D., Tang, Y. -W., Traficante, A., Vastel, C., Viti, S., Walsh, A., Wang, H., Wang, J., Ward-Thompson, D., Whitworth, A., Wilson, C. D., Xu, Y., Yang, J., Yuan, Y. -L., Yuan, L., Zavagno, A., Zhang, C., Zhang, H. -W., Zhou, C., Zhu, J. Zhou. L., Zuo, P.
We present the first release of the data and compact-source catalogue for the JCMT Large Program SCUBA-2 Continuum Observations of Pre-protostellar Evolution (SCOPE). SCOPE consists of 850-um continuum observations of 1235 Planck Galactic Cold Clumps
Externí odkaz:
http://arxiv.org/abs/1902.10180
Autor:
Tang, Mengyao, Liu, Tie, Qin, Sheng-Li, Kim, Kee-Tae, Wu, Yuefang, Tatematsu, Ken'ichi, Yuan, Jinghua, Wang, Ke, Parsons, Harriet, Koch, Patrick M., Sanhueza, Patricio, Ward-Thompson, D., Tóth, L. Viktor, Soam, Archana, Lee, Chang Won, Eden, David, Di Francesco, James, Rawlings, Jonathan, Rawlings, Mark G., Montillaud, Julien, Zhang, Chuan-Peng, Cunningham, M. R.
Planck Galactic Cold Clumps (PGCCs) possibly represent the early stages of star formation. To understand better the properties of PGCCs, we studied 16 PGCCs in the L1495 cloud with molecular lines and continuum data from Herschel, JCMT/SCUBA-2 and th
Externí odkaz:
http://arxiv.org/abs/1802.05378
The relative orientation between filamentary structures in molecular clouds and the ambient magnetic field provides insight into filament formation and stability. To calculate the relative orientation, a measurement of filament orientation is first r
Externí odkaz:
http://arxiv.org/abs/1708.01953
Different combinations of input parameters to filament identification algorithms, such as Disperse and FilFinder, produce numerous different output skeletons. The skeletons are a one pixel wide representation of the filamentary structure in the origi
Externí odkaz:
http://arxiv.org/abs/1704.06377
Autor:
Longmore, S. N., Walsh, A. J., Purcell, C. R., Burke, D. J., Henshaw, J., Walker, D., Urquhart, J., Barnes, A. T., Whiting, M., Burton, M. G., Breen, S. L., Britton, T., Brooks, K. J., Cunningham, M. R., Green, J. A., Harvey-Smith, L., Hindson, L., Hoare, M. G., Indermuehle, B., Jones, P. A., Lo, N., Lowe, V., Moore, T. J. T., Thompson, M. A., Voronkov, M. A.
The H2O Southern Galactic Plane Survey (HOPS) has mapped 100 square degrees of the Galactic plane for water masers and thermal molecular line emission using the 22-m Mopra telescope. We describe the automated spectral-line fitting pipelines used to d
Externí odkaz:
http://arxiv.org/abs/1704.03253
Autor:
Wiles, B., Lo, N., Redman, M. P., Cunningham, M. R., Jones, P. A., Burton, M. G., Bronfman, L.
Three bright molecular line sources in G333 have recently been shown to exhibit signatures of infall. We describe a molecular line radiative transfer modelling process which is required to extract the infall signature from Mopra and Nanten2 data. The
Externí odkaz:
http://arxiv.org/abs/1604.02204