Zobrazeno 1 - 10
of 530
pro vyhledávání: '"Hony, S"'
Autor:
Min, M., Bouwman, J., Dominik, C., Waters, L. B. F. M., Pontoppidan, K. M., Hony, S., Mulders, G. D., Henning, Th., van Dishoeck, E. F., Woitke, P., Evans II, Neal J., Team, The DIGIT
Context. The presence or absence of ice in protoplanetary disks is of great importance to the formation of planets. By enhancing solid surface density and increasing sticking efficiency, ice catalyzes the rapid formation of planetesimals and decrease
Externí odkaz:
http://hdl.handle.net/10150/622159
http://arizona.openrepository.com/arizona/handle/10150/622159
http://arizona.openrepository.com/arizona/handle/10150/622159
Autor:
Scicluna, P., Kemper, F., McDonald, I., Srinivasan, S., Trejo, A., Wallström, S. H. J., Wouterloot, J. G. A., Cami, J., Greaves, J., He, Jinhua, Hoai, D. T., Kim, Hyosun, Jones, O. C., Shinnaga, H., Clark, C. J. R., Dharmawardena, T., Holland, W., Imai, H., van Loon, J. Th., Menten, K. M., Wesson, R., Chawner, H., Feng, S., Goldman, S., Liu, F. C., MacIsaac, H., Tang, J., Zeegers, S., Amada, K., Antoniou, V., Bemis, A., Boyer, M. L., Chapman, S., Chen, X., Cho, S. -H., Cui, L., Dell'Agli, F., Friberg, P., Fukaya, S., Gomez, H., Gong, Y., Hadjara, M., Haswell, C., Hirano, N., Hony, S., Izumiura, H., Jeste, M., Jiang, X., Kaminski, T., Keaveney, N., Kim, J., Kraemer, K. E., Kuan, Y. -J., Lagadec, E., Lee, C. F., Li, D., Liu, S. -Y., Liu, T., de Looze, I., Lykou, F., Maraston, C., Marshall, J. P., Matsuura, M., Min, C., Otsuka, M., Oyadomari, M., Parsons, H., Patel, N. A., Peeters, E., Pham, T. A., Qiu, J., Randall, S., Rau, G., Redman, M. P., Richards, A. M. S., Serjeant, S., Shi, C., Sloan, G. C., Smith, M. W. L., Suh, K. -W., Toalá, J. A., Uttenthaler, S., Ventura, P., Wang, B., Yamamura, I., Yang, T., Yun, Y., Zhang, F., Zhang, Y., Zhao, G., Zhu, M., Zijlstra, A. A.
The Nearby Evolved Stars Survey (NESS) is a volume-complete sample of $\sim$850 Galactic evolved stars within 3\,kpc at (sub-)mm wavelengths, observed in the CO $J = $ (2$-$1) and (3$-$2) rotational lines, and the sub-mm continuum, using the James Cl
Externí odkaz:
http://arxiv.org/abs/2110.12562
Autor:
Madden, S. C., Cormier, D., Hony, S., Lebouteiller, V., Abel, N., Galametz, M., De Looze, I., Chevance, M., Polles, F. L., Lee, M. -Y., Galliano, F., Lambert-Huyghe, A., Hu, D., Ramambason, L.
Publikováno v:
A&A 643, A141 (2020)
While the CO(1-0) transition is often used to deduce the total molecular hydrogen in galaxies, it is challenging to detect in low metallicity galaxies, in spite of the star formation taking place. In contrast, the [CII] 158 micron line is relatively
Externí odkaz:
http://arxiv.org/abs/2009.00649
Autor:
Lebouteiller, V., Cormier, D., Madden, S. C., Galametz, M., Hony, S., Galliano, Frédéric, Chevance, M., Lee, Min-Young, Braine, J., Polles, F. L., Requeña-Torres, M. Angel, Indebetouw, R., Hughes, A., Abel, N.
Publikováno v:
A&A 632, A106 (2019)
(abridged) The ambiguous origin of [CII] 158um in the interstellar medium complicates its use for diagnostics concerning the star-formation rate and physical conditions in photodissociation regions (PDRs). We observed the giant HII region N11 in the
Externí odkaz:
http://arxiv.org/abs/1911.03280
Autor:
Cormier, D., Abel, N. P., Hony, S., Lebouteiller, V., Madden, S. C., Polles, F. L., Galliano, F., De Looze, I., Galametz, M., Lambert-Huyghe, A.
Publikováno v:
A&A 626, A23 (2019)
The sensitive infrared telescopes, Spitzer and Herschel, have been used to target low-metallicity star-forming galaxies, allowing us to investigate the properties of their interstellar medium (ISM) in unprecedented detail. Interpretation of the obser
Externí odkaz:
http://arxiv.org/abs/1904.08434
Autor:
Polles, F. L., Madden, S. C., Lebouteiller, V., Cormier, D., Abel, N., Galliano, F., Hony, S., Karczewski, O. L., Lee, M. -Y., Chevance, M., Galametz, M., Lianou, S.
Publikováno v:
A&A 622, A119 (2019)
Our objective is to investigate the physical properties of the ionised gas of the low-metallicity dwarf galaxy, IC 10, at various spatial scales: from individual HII regions to the entire galaxy scale and examine whether diagnostics for integrated me
Externí odkaz:
http://arxiv.org/abs/1810.03633
Autor:
Naslim, N, Tokuda, K., Onishi, T., Kemper, F., Wong, T., Morata, O., Takada, S., Harada, R., Kawamura, A., Saigo, K., Indebetouw, R., Madden, S. C., Hony, S., Meixner, M.
We present the molecular cloud properties of N55 in the Large Magellanic Cloud using $^{12}$CO(1-0) and $^{13}$CO(1-0) observations obtained with Atacama Large Millimeter Array. We have done a detailed study of molecular gas properties, to understand
Externí odkaz:
http://arxiv.org/abs/1801.01653
Autor:
Cormier, D., Bendo, G. J., Hony, S., Lebouteiller, V., Madden, S. C., Galliano, F., Glover, S. C. O., Klessen, R. S., Abel, N. P., Bigiel, F., Clark, P. C.
Properties of the cold interstellar medium of low-metallicity galaxies are not well-known due to the faintness and extremely small scale on which emission is expected. We present deep ALMA band 6 (230GHz) observations of the nearby, low-metallicity (
Externí odkaz:
http://arxiv.org/abs/1702.08467
Autor:
Min, M., Bouwman, J., Dominik, C., Waters, L. B. F. M., Pontoppidan, K. M., Hony, S., Mulders, G. D., Henning, Th., van Dishoeck, E. F., Woitke, P., Evans II, Neal J., Team, The DIGIT
The presence or absence of ice in protoplanetary disks is of great importance for the formation of planets. By enhancing the solid surface density and increasing the sticking efficiency, ice catalyzes the rapid formation of planetesimals and decrease
Externí odkaz:
http://arxiv.org/abs/1606.07266
Autor:
Chevance, M., Madden, S. C., Lebouteiller, V., Godard, B., Cormier, D., Galliano, F., Hony, S., Indebetouw, R., Bourlot, J. Le, Lee, M. Y., Petit, F. Le, Pellegrini, E., Roueff, E., Wu, R.
More complete knowledge of galaxy evolution requires understanding the process of star formation and interaction between the interstellar radiation field and the interstellar medium in galactic environments traversing a wide range of physical paramet
Externí odkaz:
http://arxiv.org/abs/1603.03573