Zobrazeno 91 - 100
of 757
pro vyhledávání: '"Bronfman, L."'
Autor:
Schuller, F., Menten, K. M., Contreras, Y., Wyrowski, F., Schilke, P., Bronfman, L., Henning, T., Walmsley, C. M., Beuther, H., Bontemps, S., Cesaroni, R., Deharveng, L., Garay, G., Herpin, F., Lefloch, B., Linz, H., Mardones, D., Minier, V., Molinari, S., Motte, F., Nyman, L. -A., Reveret, V., Risacher, C., Russeil, D., Schneider, N., Testi, L., Troost, T., Vasyunina, T., Wienen, M., Zavagno, A., Kovacs, A., Kreysa, E., Siringo, G., Weiss, A.
(Abridged) Studying continuum emission from interstellar dust is essential to locating and characterizing the highest density regions in the interstellar medium. In particular, the early stages of massive star formation remain poorly understood. Our
Externí odkaz:
http://arxiv.org/abs/0903.1369
Autor:
Sievers, J. L., Mason, B. S., Weintraub, L., Achermann, C., Altamirano, P., Bond, J. R., Bronfman, L., Bustos, R., Contaldi, C., Dickinson, C., Jones, M. E., May, J., Myers, S. T., Oyarce, N., Padin, S., Pearson, T. J., Pospieszalski, M., Readhead, A. C. S., Reeves, R., Shepherd, M. C., Taylor, A. C., Torres, S.
We present final results on the angular power spectrum of total intensity anisotropies in the CMB from the CBI. Our analysis includes all primordial anisotropy data collected between January 2000 and April 2005, and benefits significantly from an imp
Externí odkaz:
http://arxiv.org/abs/0901.4540
IRAS19410+2336 is a young massive star forming region with an intense outflow activity. We present here spatially resolved NIR spectroscopy which allows us to verify whether the H2 emission detected in this object originates from thermal emission in
Externí odkaz:
http://arxiv.org/abs/0807.5099
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Pineda, J. L., Mizuno, N., Stutzki, J., Cubick, M., Aravena, M., Bensch, F., Bertoldi, F., Bronfman, L., Fujishita, K., Graf, U. U., Hitschfeld, M., Honingh, N., Jakob, H., Jacobs, K., Kawamura, A., Klein, U., Kramer, C., May, J., Miller, M., Mizuno, Y., Müller, P., Onishi, T., Ossenkopf, V., Rabanus, D., Röllig, M., Rubio, M., Sasago, H., Schieder, R., Simon, R., Sun, K., Volgenau, N., Yamamoto, H., Fukui, Y.
Star formation at earlier cosmological times takes place in an interstellar medium with low metallicity. The Large Magellanic Cloud (LMC) is ideally suited to study star formation in such an environment. The physical and chemical state of the ISM in
Externí odkaz:
http://arxiv.org/abs/0802.1929
We report millimeter interferometric observations of polarized continuum and line emission from the massive star forming region G34.4. Polarized thermal dust emission at 3 mm wavelength and CO $J=1 \to 0$ line emission were observed using the Berkele
Externí odkaz:
http://arxiv.org/abs/0801.4316
Autor:
Hitschfeld, M., Aravena, M., Kramer, C., Bertoldi, F., Stutzki, J., Bensch, F., Bronfman, L., Cubick, M., Fujishita, M., Fukui, Y., Graf, U. U., Honingh, N., Ito, S., Jakob, H., Jacobs, K., Klein, U., Koo, B. -C., May, J., Miller, M., Miyamoto, Y., Mizuno, N., Onishi, T., Park, Y. -S., Pineda, J. L., Rabanus, D., Roellig, M., Sasago, H., Schieder, R., Simon, R., Sun, K., Volgenau, N., Yamamoto, H., Yonekura, Y.
Studying molecular gas in the central regions of the star burst galaxies NGC4945 and Circinus enables us to characterize the physical conditions and compare them to previous local and high-z studies. We estimate temperature, molecular density and col
Externí odkaz:
http://arxiv.org/abs/0712.1924
Autor:
Kramer, C., Cubick, M., Roellig, M., Sun, K., Yonekura, Y., Aravena, M., Bensch, F., Benz, A., Bertoldi, F., Bronfman, L., Fujishita, M., Fukui, Y., Graf, U. U., Hitschfeld, M., Honingh, N., Ito, S., Jakob, H., Jacobs, K., Klein, U., Koo, B. -C., May, J., Miller, M., Miyamoto, Y., Mizuno, N., Onishi, T., Park, Y. -S., Pineda, J. L., Rabanus, D., Sasago, H., Schieder, R., Simon, R., Stutzki, J., Volgenau, N., Yamamoto, H.
The Carina region is an excellent astrophysical laboratory for studying the feedback mechanisms of newly born, very massive stars within their natal giant molecular clouds (GMCs) at only 2.35 kpc distance. We use a clumpy PDR model to analyse the obs
Externí odkaz:
http://arxiv.org/abs/0711.1320
Autor:
Shepherd, D. S., Povich, M. S., Whitney, B. A., Robitaille, T. P., Nurnberger, D. E. A., Bronfman, L., Stark, D. P., Indebetouw, R., Meade, M. R., Babler, B. L.
Publikováno v:
Astrophys.J.669:464-482,2007
We have observed the central region of the IR-dark cloud filament associated with IRAS 18507+0121 at millimeter wavelengths in CO(1-0), 13CO(1-0), and C18O(1-0) line emission and with the Spitzer Space Telescope at mid-IR wavelengths. Five massive ou
Externí odkaz:
http://arxiv.org/abs/0706.4330
Aims. Motivated by the new determination of the distance to the microquasar GRO J1655-40 by Foellmi et al. (2006), we conduct a detailed study of the distribution of the atomic and molecular gas, and dust around the open cluster NGC 6242, the possibl
Externí odkaz:
http://arxiv.org/abs/astro-ph/0703674