Zobrazeno 1 - 10
of 2 171
pro vyhledávání: '"Kurtz, S."'
G34.26+0.15 is a region of high-mass star formation that contains a broad range of young stellar objects in different stages of evolution, including a hot molecular core, hyper-compact HII regions and a prototypical cometary ultra-compact HII region.
Externí odkaz:
http://arxiv.org/abs/2306.07394
The study of the interaction between ionized jets, molecular outflows and their environments is critical to understanding high-mass star formation, especially because jets and outflows are thought to be key in the transfer of angular momentum outward
Externí odkaz:
http://arxiv.org/abs/2306.00111
Autor:
Rojas-García, O. S., Gómez-Ruiz, A. I., Palau, A., Orozco-Aguilera, M. T., Kurtz, S. E., Dagostino, M. Chavez
G351.16+0.70 is a relatively well-studied High Mass Star Forming Region with at least two main bipolar outflow structures originating from an OB embedded star and multiple IR cores. Using high-resolution and large bandwidth SMA observations, we studi
Externí odkaz:
http://arxiv.org/abs/2303.02527
Autor:
Irabor, T., Hoare, M. G., Burton, M., Cotton, W. D., Diamond, P., Dougherty, S., Ellingsen, S. P., Fender, R., Fuller, G. A., Garrington, S., Goldsmith, P. F., Green, J., Gunn, A. G., Jackson, J., Kurtz, S., Lumsden, S. L., Marti, J., McDonald, I., Molinari, S., Moore, T. J., Mutale, M., Muxlow, T., OBrien, T., Oudmaijer, R. D., Paladini, R., Pandian, J. D., Paredes, J. M., Richards, A. M. S., Sanchez-Monge, A., Spencer, R., Thompson, M. A., Umana, G., Urquhart, J. S., Wieringa, M., Zijlstra, A.
We present the first high spatial resolution radio continuum survey of the southern Galactic plane. The CORNISH project has mapped the region defined by $295^{\circ} < l < 350^{\circ}$; $|b| < 1^{\circ}$ at 5.5-GHz, with a resolution of 2.5$^{''}$ (F
Externí odkaz:
http://arxiv.org/abs/2301.01988
Autor:
Rojas-García, O. S., Gómez-Ruiz, A. I., Palau, A., Orozco-Aguilera, M. T., Dagostino, M. Chavez, Kurtz, S. E.
The interstellar medium contains dust and gas, in which at high densities and cold conditions molecules can proliferate. Interstellar Complex Organic Molecules (iCOMs) are C-bearing species that contain at least six atoms. As they are detected in you
Externí odkaz:
http://arxiv.org/abs/2207.09426
Autor:
Bayandina, O. S., Brogan, C. L., Burns, R. A., Garatti, A. Caratti o, Chibueze, J. O., Heever, S. P. van den, Kurtz, S. E., MacLeod, G. C., Moscadelli, L., Sobolev, A. M., Sugiyama, K., Val'tts, I. E., Yonekura, Y.
Publikováno v:
A&A 664, A44 (2022)
The massive young stellar object (MYSO) G358.93-0.03-MM1 showed an extraordinary near-infrared- to (sub-)millimetre-dark and far-infrared-loud accretion burst, which is closely associated with flares of several class II methanol maser transitions, an
Externí odkaz:
http://arxiv.org/abs/2206.12119
Autor:
Bayandina, O. S., Brogan, C. L., Burns, R. A., Chen, X., Hunter, T. R., Kurtz, S. E., MacLeod, G. C., Sobolev, A. M., Sugiyama, K., Val'tts, I. E., Yonekura, Y.
Publikováno v:
The Astronomical Journal, 163:83 (16pp), 2022 February
We present the most complete to date interferometric study of the centimeter wavelength methanol masers detected in G358.93-0.03 at the burst and post-burst epochs. A unique, NIR/(sub)mm-dark and FIR-loud MYSO accretion burst was recently discovered
Externí odkaz:
http://arxiv.org/abs/2201.12075
Autor:
Dewangan, L. K., Zinchenko, I. I., Zemlyanukha, P. M., Liu, S. -Y., Su, Y. -N., Kurtz, S. E., Ojha, D. K., Pazukhin, A. G., Mayya, Y. D.
We present line and continuum observations (resolution ~0.3"-3.5") made with the Atacama Large Millimeter/submillimeter Array (ALMA), Submillimeter Array, and Very Large Array of a young O-type protostar W42-MME (mass: 19-4 Msun). The ALMA 1.35 mm co
Externí odkaz:
http://arxiv.org/abs/2111.01373
Autor:
M., T., Rodríguez, Hofner, P., Araya, E. D., Zhang, Q., Linz, H., Kurtz, S., Gómez, L., Carrasco-González, C., Rosero, V.
We present Very Large Array C, X, and Q-band continuum observations, as well as 1.3 mm continuum and CO(2-1) observations with the Submillimeter Array toward the high-mass protostellar candidate ISOSS J23053+5953 SMM2. Compact cm continuum emission w
Externí odkaz:
http://arxiv.org/abs/2109.01243
Autor:
Shuvo, Onic I., Araya, E. D., Tan, W. S., Hofner, P., Kurtz, S., Pihlstrom, Y. M., Hoffman, I. M.
Spectral lines from formaldehyde (H2CO) molecules at cm wavelengths are typically detected in absorption and trace a broad range of environments, from diffuse gas to giant molecular clouds. In contrast, thermal emission of formaldehyde lines at cm wa
Externí odkaz:
http://arxiv.org/abs/2103.14492