Zobrazeno 51 - 60
of 757
pro vyhledávání: '"Bronfman, L."'
Autor:
QUIET Collaboration, Ruud, T. M., Fuskeland, U., Wehus, I. K., Vidal, M., Araujo, D., Bischoff, C., Buder, I., Chinone, Y., Cleary, K., Dumoulin, R. N., Kusaka, A., Monsalve, R., Naess, S. K., Newburgh, L. B., Reeves, R. A., Zwart, J. T. L., Bronfman, L., Davies, R. D., Davis, R., Dickinson, C., Eriksen, H. K., Gaier, T., Gundersen, J. O., Hasegawa, M., Hazumi, M., Huffenberger, K. M., Jones, M. E., Lawrence, C. R., Leitch, E. M., Limon, M., Miller, A. D., Pearson, T. J., Piccirillo, L., Radford, S. J. E., Readhead, A. C. S., Samtleben, D., Seiffert, M., Shepherd, M. C., Staggs, S. T., Tajima, O., Thompson, K. L.
Publikováno v:
ApJ 811, 89 (2015)
We present polarization observations of two Galactic plane fields centered on Galactic coordinates (l,b)=(0 deg,0 deg) and (329 deg, 0 deg) at Q- (43 GHz) and W-band (95 GHz), covering between 301 and 539 square degrees depending on frequency and fie
Externí odkaz:
http://arxiv.org/abs/1508.02778
Autor:
Giannetti, A., Wyrowski, F., Leurini, S., Urquhart, J., Csengeri, T., Menten, K. M., Bronfman, L., van der Tak, F. F. S.
Context: Infrared dark clouds are the coldest and densest portions of giant molecular clouds. The most massive ones represent some of the most likely birthplaces for the next generation of massive stars in the Milky Way. Because a strong mid-IR backg
Externí odkaz:
http://arxiv.org/abs/1507.05808
Autor:
Wienen, M., Wyrowski, F., Menten, K. M., Urquhart, J. S., Csengeri, T., Walmsley, C. M., Bontemps, S., Russeil, D., Bronfman, L., Koribalski, B. S., Schuller, F.
The formation of high mass stars and clusters occurs in giant molecular clouds. Objects in evolved stages of massive star formation such as protostars, hot molecular cores, and ultracompact HII regions have been studied in more detail than earlier, c
Externí odkaz:
http://arxiv.org/abs/1503.00007
Autor:
Lo, N., Cunningham, M. R., Jones, P. A., Bronfman, L., Cortes, P. C., Simon, R., Lowe, V., Fissel, L., Novak, G.
We present first results of neutral carbon ([CI], 3P1 - 3P0 at 492 GHz) and carbon monoxide (13CO, J = 1 - 0) mapping in the Vela Molecular Ridge cloud C (VMR-C) and G333 giant molecular cloud complexes with the NANTEN2 and Mopra telescopes. For the
Externí odkaz:
http://arxiv.org/abs/1412.0476
Autor:
Urquhart, J. S., Csengeri, T., Wyrowski, F., Schuller, F., Bontemps, S., Bronfman, L., Menten, K. M., Walmsley, C. M., Contreras, Y., Beuther, H., Wienen, M., Linz, H.
Publikováno v:
A&A 568, A41 (2014)
The APEX Telescope Large Area Survey of the Galaxy (ATLASGAL) is the largest and most sensitive systematic survey of the inner Galactic plane in the submillimetre wavelength regime. The observations were carried out with the Large APEX Bolometer Came
Externí odkaz:
http://arxiv.org/abs/1406.5741
Autor:
Urquhart, J. S., Moore, T. J. T., Csengeri, T., Wyrowski, F., Schuller, F., Hoare, M. G., Lumsden, S. L., Mottram, J. C., Thompson, M. A., Menten, K. M., Walmsley, C. M., Bronfman, L., Pfalzner, S., König, C., Wienen, M.
By matching infrared-selected, massive young stellar objects (MYSOs) and compact HII regions in the RMS survey to massive clumps found in the submillimetre ATLASGAL survey, we have identified ~1000 embedded young massive stars between 280\degr < $\el
Externí odkaz:
http://arxiv.org/abs/1406.5078
The Columbia - U. de Chile CO Survey of the Southern Milky Way is used for separating the CO(1-0) emission of the fourth Galactic quadrant within the solar circle into its dominant components, giant molecular clouds (GMCs). After the subtraction of a
Externí odkaz:
http://arxiv.org/abs/1402.6359
We are presenting here a follow-up study of the molecular gas and dust in the environs of the star forming region NGC 3503. This study aims at dealing with the interaction of NGC 3503 with its parental molecular cloud, and also with the star formatio
Externí odkaz:
http://arxiv.org/abs/1402.5041
Autor:
Csengeri, T., Urquhart, J. S., Schuller, F., Motte, F., Bontemps, S., Wyrowski, F., Menten, K. M., Bronfman, L., Beuther, H., Henning, Th., Testi, L., Zavagno, A., Walmsley, M.
The formation processes and the evolutionary stages of high-mass stars are poorly understood compared to low-mass stars. Large-scale surveys are needed to provide an unbiased census of high column density sites which can potentially host precursors t
Externí odkaz:
http://arxiv.org/abs/1312.0937
Autor:
Eckart, Andreas, Horrobin, M., Britzen, S., Zamaninasab, M., Muzic, K., Sabha, N., Shahzamanian, B., Yazici, S., Moser, L., Garcia-Mari, M., Valencia-S., M., Borkar, A., Bursa, M., Karssen, G., Karas, V., Zajacek, M., Bronfman, L., Finger, R., Jalali, B., Vitale, M., Rauch, C., Kunneriath, D., Moultaka, J., Straubmeier, C., Rashed, Y. E., Markakis, K., Zensus, A.
A fast moving infrared excess source (G2) which is widely interpreted as a core-less gas and dust cloud approaches Sagittarius A* (SgrA*) on a presumably elliptical orbit. VLT K_s-band and Keck K'-band data result in clear continuum identifications a
Externí odkaz:
http://arxiv.org/abs/1311.2753