Zobrazeno 1 - 10
of 643
pro vyhledávání: '"Eden, D."'
Autor:
Eden, D. J., Liu, Tie, Moore, T. J. T., Di Francesco, J., Fuller, G., Kim, Kee-Tae, Li, Di, Liu, S. -Y., Plume, R., Tatematsu, Ken'ichi, Thompson, M. A., Wu, Y., Bronfman, L., Butner, H. M., Currie, M. J., Garay, G., Goldsmith, P. F., Hirano, N., Johnstone, D., Juvela, M., Lai, S. -P., Lee, C. W., Mannfors, E. E., Olguin, F., Pattle, K., Park, Geumsook, Polychroni, D., Rawlings, M., Rigby, A. J., Sanhueza, P., Traficante, A., Urquhart, J. S., Weferling, B., White, G. J., Yadav, R. K.
We have investigated the physical properties of Planck Galactic Cold Clumps (PGCCs) located in the Galactic Plane, using the JCMT Plane Survey (JPS) and the SCUBA-2 Continuum Observations of Pre-protostellar Evolution (SCOPE) survey. By utilising a s
Externí odkaz:
http://arxiv.org/abs/2405.00493
Autor:
Ge, Y., Wang, K., Duarte-Cabral, A., Pettitt, A. R., Dobbs, C. L., Sánchez-Monge, Á., Neralwar, K. R., Urquhart, J. S., Colombo, D., Durán-Camacho, E., Beuther, H., Bronfman, L., Rigby, A. J., Eden, D., Neupane, S., Barnes, P., Henning, T., Yang, A. Y.
Publikováno v:
A&A 675, A119 (2023)
Context. Filamentary structures in the interstellar medium are closely related to star formation. Dense gas mass fraction (DGMF) or clump formation efficiency in large-scale filaments possibly determine their hosting star formation activities. Aims.
Externí odkaz:
http://arxiv.org/abs/2305.07353
Autor:
Elia, D., Molinari, S., Schisano, E., Soler, J. D., Merello, M., Russeil, D., Veneziani, M., Zavagno, A., Noriega-Crespo, A., Olmi, L., Benedettini, M., Hennebelle, P., Klessen, R. S., Leurini, S., Paladini, R., Pezzuto, S., Traficante, A., Eden, D. J., Martin, P. G., Sormani, M., Coletta, A., Colman, T., Plume, R., Maruccia, Y., Mininni, C., Liu, S. J.
We present a new derivation of the Milky Way's current star formation rate (SFR) based on the data of the Hi-GAL Galactic plane survey. We estimate the distribution of the SFR across the Galactic plane from the star-forming clumps identified in the H
Externí odkaz:
http://arxiv.org/abs/2211.05573
Autor:
Wells, M. R. A., Urquhart, J. S., Moore, T. J. T., Browning, K. E., Ragan, S. E., Rigby, A. J., Eden, D. J., Thompson, M. A.
The ATLASGAL survey has characterised the properties of approximately 1000 embedded HII regions and found an empirical relationship between the clump mass and bolometric luminosity that covers 3-4 orders of magnitude. Comparing this relation with sim
Externí odkaz:
http://arxiv.org/abs/2208.11121
Autor:
Neralwar, K. R., Colombo, D., Duarte-Cabral, A., Urquhart, J. S., Mattern, M., Wyrowski, F., Menten, K. M., Barnes, P., Sanchez-Monge, A., Rigby, A. J., Mazumdar, P., Eden, D., Csengeri, T., Dobbs, C. L., Veena, V. S., Neupane, S., Henning, T., Schuller, F., Leurini, S., Wienen, M., Yang, A. Y., Ragan, S. E., Medina, S., Nguyen-Luong, Q.
Publikováno v:
A&A 664, A84 (2022)
The Structure, Excitation, and Dynamics of the Inner Galactic InterStellar Medium (SEDIGISM) survey has produced high (spatial and spectral) resolution $^{13}$CO (2-1) maps of the Milky Way. It has allowed us to investigate the molecular interstellar
Externí odkaz:
http://arxiv.org/abs/2205.02253
Autor:
Neralwar, K. R., Colombo, D., Duarte-Cabral, A., Urquhart, J. S., Mattern, M., Wyrowski, F., Menten, K. M., Barnes, P., Sanchez-Monge, A., Beuther, H., Rigby, A. J., Mazumdar, P., Eden, D., Csengeri, T., Dobbs, C. L., Veena, V. S., Neupane, S., Henning, T., Schuller, F., Leurini, S., Wienen, M., Yang, A. Y., Ragan, S. E., Medina, S., Nguyen-Luong, Q.
Publikováno v:
A&A 663, A56 (2022)
We present one of the very first extensive classifications of a large sample of molecular clouds based on their morphology. This is achieved using a recently published catalogue of 10663 clouds obtained from the first data release of the SEDIGISM sur
Externí odkaz:
http://arxiv.org/abs/2203.02504
Autor:
Urquhart, J. S., Wells, M. R. A., Pillai, T., Leurini, S., Giannetti, A., Moore, T. J. T., Thompson, M. A., Figura, C., Colombo, D., Yang, A. Y., Koenig, C., Wyrowski, F., Menten, K. M., Rigby, A. J., Eden, D. J., Ragan, S. E.
ATLASGAL is a 870-mircon dust survey of 420 square degrees of the inner Galactic plane and has been used to identify ~10 000 dense molecular clumps. Dedicated follow-up observations and complementary surveys are used to characterise the physical prop
Externí odkaz:
http://arxiv.org/abs/2111.12816
Autor:
Yang, A. Y., Urquhart, J. S., Wyrowski, F., Thompson, M. A., König, C., Colombo, D., Menten, K. M., Duarte-Cabral, A., Schuller, F., Csengeri, T., Eden, D., Barnes, P., Traficante, A., Bronfman, L., Sanchez-Monge, A., Ginsburg, A., Cesaroni, R., Lee, M. -Y., Beuther, H., Medina, S. -N. X., Mazumdar, P., Henning, T.
Publikováno v:
A&A 658, A160 (2022)
Context. The formation processes of massive stars are still unclear but a picture is emerging involving accretion disks and molecular outflows in what appears to be a scaled-up version of low-mass star formation. A census of outflow activity towards
Externí odkaz:
http://arxiv.org/abs/2111.10850
Autor:
Colombo, D., Duarte-Cabral, A., Pettitt, A. R., Urquhart, J. S., Wyrowski, F., Csengeri, T., Neralwar, K. R., Schuller, F., Menten, K. M., Anderson, L., Barnes, P., Beuther, H., Bronfman, L., Eden, D., Ginsburg, A., Henning, T., Koenig, C., Lee, M. -Y., Mattern, M., Medina, S., Ragan, S. E., Rigby, A. J., Sanchez-Monge, A., Traficante, A., Yang, A. Y., Wienen, M.
Publikováno v:
A&A 658, A54 (2022)
The morphology of the Milky Way is still a matter of debate. In order to shed light on uncertainties surrounding the structure of the Galaxy, in this paper, we study the imprint of spiral arms on the distribution and properties of its molecular gas.
Externí odkaz:
http://arxiv.org/abs/2110.06071
Autor:
Mannfors, E., Juvela, M., Bronfman, L., Eden, D. J., He, Jinhua, Kim, Gwanjeon, Kim, Kee-Tae, Kirppu, H., Liu, T., Montillaud, J., Parsons, H., Sanhueza, Patricio, Shang, Hsien, Soam, A., Tatematsu, K., Traficante, A., Väisälä, M. S., Lee, Chang Won
Publikováno v:
A&A 654, A123 (2021)
We aim to characterize a diverse selection of dense, potentially star-forming cores, clumps, and clouds within the Milky Way in terms of their dust emission and SF activity. We studied 53 fields that have been observed in the JCMT SCUBA-2 continuum s
Externí odkaz:
http://arxiv.org/abs/2106.10114