Zobrazeno 1 - 10
of 1 569
pro vyhledávání: '"Jacobs, K. A."'
Autor:
Bonne, L., Kabanovic, S., Schneider, N., Zavagno, A., Keilmann, E., Simon, R., Buchbender, C., Guesten, R., Jacob, A. M., Jacobs, K., Kavak, U., Polles, F. L., Tiwari, M., Wyrowski, F., Tielens, A. G. G. M
Publikováno v:
A&A 679, L5 (2023)
It has long been discussed whether stellar feedback in the form of winds and/or radiation can shred the nascent molecular cloud, thereby controlling the star formation rate. However, directly probing and quantifying the impact of stellar feedback on
Externí odkaz:
http://arxiv.org/abs/2310.01657
Autor:
Schneider, N., Simon, R., Guevara, C., Buchbender, C., Higgins, R. D., Okada, Y., Stutzki, J., Guesten, R., Anderson, L. D., Bally, J., Beuther, H., Bonne, L., Bontemps, S., Chambers, E., Csengeri, T., Graf, U. U., Gusdorf, A., Jacobs, K., Kabanovic, S., Karim, R., Luisi, M., Menten, K., Mertens, M., Mookerjea, B., Ossenkopf-Okada, V., Pabst, C., Pound, M. W., Richter, H., Reyes, N., Ricken, O., Roellig, M., Russeil, D., Sanchez-Monge, A., Sandell, G., Tiwari, M., Wiesemeyer, H., Wolfire, M., Wyrowski, F., Zavagno, A., Tielens, A. G. G. M.
Publikováno v:
PASP 2020, Volume 132, Number 1016; https://iopscience.iop.org/article/10.1088/1538-3873/aba840
FEEDBACK is a SOFIA legacy program dedicated to study the interaction of massive stars with their environment. It performs a survey of 11 galactic high mass star forming regions in the 158 $\mu$m (1.9 THz) line of CII and the 63 $\mu$m (4.7 THz) line
Externí odkaz:
http://arxiv.org/abs/2009.08730
Akademický článek
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Akademický článek
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Autor:
Risacher, C., Güsten, R., Stutzk, J., Hübers, H. -W., Aladro, R., Bell, A., Buchbender, C., Büchel, D., Csengeri, T., Duran, C., Graf, U. U., Higgins, R. D., Honingh, C. E., Jacobs, K., Justen, M., Klein, B., Mertens, M., Okada, Y., Parikka, A., Pütz, P., Reyes, N., Richter, H., Ricken, O., Riquelme, D., Rothbart, N., Schneider, N., Simon, R., Wienold, M., Wiesemeyer, H., Ziebart, M., Fusco, P., Rosner, S., Wohler, B.
We present the performance of the upGREAT heterodyne array receivers on the SOFIA telescope after several years of operations. This instrument is a multi-pixel high resolution (R > 10^7) spectrometer for the Stratospheric Observatory for Far-Infrared
Externí odkaz:
http://arxiv.org/abs/1812.07403
Autor:
Leung, N., Lu, Y., Chakram, S., Naik, R. K., Earnest, N., Ma, R., Jacobs, K., Cleland, A. N., Schuster, D. I.
We propose and experimentally demonstrate a simple and efficient scheme for photonic communication between two remote superconducting modules. Each module consists of a random access quantum information processor with eight-qubit multimode memory and
Externí odkaz:
http://arxiv.org/abs/1804.02028
Autor:
Langer, W. D., Velusamy, T., Goldsmith, P. F., Pineda, J. L., Chambers, E. T., Sandell, G., Risacher, C., Jacobs, K.
Determining the properties of the warm ionized medium (WIM) at the leading edge of spiral arms is important for understanding its dynamics and cloud formation. The inner edge of the Scutum arm tangency is a unique location in which to disentangle the
Externí odkaz:
http://arxiv.org/abs/1708.02310
Autor:
Gusdorf, A., Anderl, S., Lefloch, B., Leurini, S., Wiesemeyer, H., Guesten, R., Benedettini, M., Codella, C., Godard, B., Gomez-Ruiz, A. I., Jacobs, K., Kristensen, L. E., Lesaffre, P., Forets, G. Pineau des, Lis, D. C.
Publikováno v:
A&A 602, A8 (2017)
Protostellar jets and outflows are key features of the star-formation process, and primary processes of the feedback of young stars on the interstellar medium. Understanding the underlying shocks is necessary to explain how jets and outflows are laun
Externí odkaz:
http://arxiv.org/abs/1704.03796
Autor:
Risacher, C., Guesten, R., Stutzki, J., Huebers, H. -W., Bell, A., Buchbender, C., Buechel, D., Csengeri, T., Graf, U. U., Heyminck, S., Higgins, R. D., Honingh, C. E., Jacobs, K., Klein, B., Okada, Y., Parikka, A., Puetz, P., Reyes, N., Ricken, O., Riquelme, D., Simon, R., Wiesemeyer, H.
Publikováno v:
A&A 595, A34 (2016)
We present a new multi-pixel high resolution (R >10^7) spectrometer for the Stratospheric Observatory for Far-Infrared Astronomy (SOFIA). The receiver uses 2 x 7-pixel subarrays in orthogonal polarization, each in an hexagonal array around a central
Externí odkaz:
http://arxiv.org/abs/1607.04239
Publikováno v:
A&A 591, A33 (2016)
Aims: We investigate how much of the [CII] emission in the nucleus of the nearby spiral galaxy IC 342 is contributed by PDRs and by the ionized gas. We examine the spatial variations of starburst/PDR activity and study the correlation of the [CII] li
Externí odkaz:
http://arxiv.org/abs/1604.07362