Zobrazeno 1 - 10
of 30
pro vyhledávání: '"Sadavoy, S. I."'
Autor:
Kirk, H., Dunham, M. M., Francesco, J. Di, Johnstone, D., Offner, S. S. R., Sadavoy, S. I., Tobin, J. J., Arce, H. G., Bourke, T. L., Mairs, S., Myers, P. C., Pineda, J. E., Schnee, S., Shirley, Y. L.
Compact substructure is expected to arise in a starless core as mass becomes concentrated in the central region likely to form a protostar. Additionally, multiple peaks may form if fragmentation occurs. We present Atacama Large Millimeter/submillimet
Externí odkaz:
http://hdl.handle.net/10150/624012
http://arizona.openrepository.com/arizona/handle/10150/624012
http://arizona.openrepository.com/arizona/handle/10150/624012
Autor:
collaboration, CCAT-Prime, Aravena, M., Austermann, J. E., Basu, K., Battaglia, N., Beringue, B., Bertoldi, F., Bigiel, F., Bond, J. R., Breysse, P. C., Broughton, C., Bustos, R., Chapman, S. C., Charmetant, M., Choi, S. K., Chung, D. T., Clark, S. E., Cothard, N. F., Crites, A. T., Dev, A., Douglas, K., Duell, C. J., Dunner, R., Ebina, H., Erler, J., Fich, M., Fissel, L. M., Foreman, S., Gallardo, P. A., Gao, J., García, Pablo, Giovanelli, R., Golec, J. E., Groppi, C. E., Haynes, M. P., Henke, D., Hensley, B., Herter, T., Higgins, R., Hlozek, R., Huber, A., Huber, Z., Hubmayr, J., Jackson, R., Johnstone, D., Karoumpis, C., Keating, L. C., Komatsu, E., Li, Y., Magnelli, B., Matthews, B. C., Mauskopf, P., McMahon, J. J., Meerburg, P. D., Meyers, J., Muralidhara, V., Murray, N. W., Niemack, M. D., Nikola, T., Okada, Y., Puddu, R., Riechers, D. A., Rosolowsky, E., Rossi, K., Rotermund, K., Roy, A., Sadavoy, S. I., Schaaf, R., Schilke, P., Scott, D., Simon, R., Sinclair, Adrian K., Sivakoff, G. R., Stacey, G. J., Stutz, Amelia M., Stutzki, J., Tahani, M., Thanjavur, K., Timmermann, R. A., Ullom, J. N., van Engelen, A., Vavagiakis, E. M., Vissers, M. R., Wheeler, J. D., White, S. D. M., Zhu, Y., Zou, B.
We present a detailed overview of the science goals and predictions for the Prime-Cam direct detection camera/spectrometer being constructed by the CCAT-prime collaboration for dedicated use on the Fred Young Submillimeter Telescope (FYST). The FYST
Externí odkaz:
http://arxiv.org/abs/2107.10364
Autor:
Lippok, N., Launhardt, R., Henning, Th., Beuther, Z. Balog. H., Kainulainen, J., Krause, O., Linz, H., Nielbock, M., Ragan, S. E., Robitaille, T. P., Sadavoy, S. I., Schmiedeke, A.
Publikováno v:
A&A 592, A61 (2016)
Constraining the temperature and density structure of dense molecular cloud cores is fundamental for understanding the initial conditions of star formation. We use Herschel observations of the thermal FIR dust emission from nearby isolated molecular
Externí odkaz:
http://arxiv.org/abs/1606.04318
We present new measurements of the dust emissivity index, beta, for the high-mass, star-forming OMC 2/3 filament. We combine 160-500 um data from Herschel with long-wavelength observations at 2 mm and fit the spectral energy distributions across a ~
Externí odkaz:
http://arxiv.org/abs/1601.06769
Autor:
Konyves, V., Andre, Ph., Men'shchikov, A., Palmeirim, P., Arzoumanian, D., Schneider, N., Roy, A., Didelon, P., Maury, A., Shimajiri, Y., Di Francesco, J., Bontemps, S., Peretto, N., Benedettini, M., Bernard, J. -Ph., Elia, D., Griffin, M. J., Hill, T., Kirk, J., Ladjelate, B., Marsh, K., Martin, P. G., Motte, F., Luong, Q. Nguyen, Pezzuto, S., Roussel, H., Rygl, K. L. J., Sadavoy, S. I., Schisano, E., Spinoglio, L., Ward-Thompson, D., White, G. J.
Publikováno v:
A&A 584, A91 (2015)
We present and discuss the results of the Herschel Gould Belt survey observations in a ~11 deg^2 area of the Aquila molecular cloud complex at d~260 pc, imaged with the SPIRE/PACS cameras from 70 to 500 micron. We identify a complete sample of starle
Externí odkaz:
http://arxiv.org/abs/1507.05926
Autor:
Sadavoy, S. I., Di Francesco, J., Andre, Ph., Pezzuto, S., Bernard, J. -P., Maury, A., Men'shchikov, A., Motte, F., Nguyen-Luong, Q., Schneider, N., Arzoumanian, D., Benedettini, M., Bontemps, S., Elia, D., Hennemann, M., Hill, T., Konyves, V., Louvet, F., Peretto, N., Roy, A., White, G. J.
We use PACS and SPIRE continuum data at 160 um, 250 um, 350 um, and 500 um from the Herschel Gould Belt Survey to sample seven clumps in Perseus: B1, B1-E, B5, IC348, L1448, L1455, and NGC1333. Additionally, we identify and characterize the embedded
Externí odkaz:
http://arxiv.org/abs/1404.7142
Autor:
Kirk, J. M., Ward-Thompson, D., Palmeirim, P., Andre, Ph., Griffin, M. J., Hargrave, P. J., Konyves, V., Bernard, J. P., Nutter, D. J., Sibthorpe, B., Di Francesco, J., Abergel, A., Arzoumanian, D., Benedettini, M., Bontemps, S., Elia, D., Hennemann, M., Hill, T., Men'shchikov, A., Motte, F., Nguyen-Luong, Q., Peretto, N., Pezzuto, S., Rygl, K. L. J., Sadavoy, S. I., Schisano, E., Schneider, N., Testi, L., White, G.
The whole of the Taurus region (a total area of 52 sq. deg.) has been observed by the Herschel SPIRE and PACS instruments at wavelengths of 70, 160, 250, 350 and 500 {\mu}m as part of the Herschel Gould Belt Survey. In this paper we present the first
Externí odkaz:
http://arxiv.org/abs/1304.4098
Autor:
Sadavoy, S. I., Di Francesco, J., Johnstone, D., Currie, M. J., Drabek, E., Hatchell, J., Nutter, D., André, Ph., Arzoumanian, D., Benedettini, M., Bernard, J. -P., Duarte-Cabral, A., Fallscheer, C., Friesen, R., Greaves, J., Hennemann, M., Hill, T., Jenness, T., Könyves, V., Matthews, B., Mottram, J. C., Pezzuto, S., Roy, A., Rygl, K., Schneider-Bontemps, N., Spinoglio, L., Testi, L., Tothill, N., Ward-Thompson, D., White, G.
We present Herschel observations from the Herschel Gould Belt Survey and SCUBA-2 science verification observations from the JCMT Gould Belt Survey of the B1 clump in the Perseus molecular cloud. We determined the dust emissivity index using four diff
Externí odkaz:
http://arxiv.org/abs/1303.1529
Autor:
Rivera-Ingraham, A., Martin, P. G., Polychroni, D., Motte, F., Schneider, N., Bontemps, S., Hennemann, M., Menshchikov, A., Luong, Q. Nguyen, Andre, Ph., Arzoumanian, D., Bernard, J. -Ph., Di Francesco, J., Elia, D., Fallscheer, C., Hill, T., Li, J. Z., Minier, V., Pezzuto, S., Roy, A., Rygl, K. L. J., Sadavoy, S. I., Spinoglio, L., White, G. J., Wilson, C. D.
The W3 GMC is a prime target for the study of the early stages of high-mass star formation. We have used Herschel data from the HOBYS key program to produce and analyze column density and temperature maps. Two preliminary catalogs were produced by ex
Externí odkaz:
http://arxiv.org/abs/1301.3805
Autor:
Sadavoy, S. I., Di Francesco, J., Andre, Ph., Pezzuto, S., Bernard, J. -P., Bontemps, S., Bressert, E., Chitsazzadeh, S., Fallscheer, C., Hennemann, M., Hill, T., Martin, P., Motte, F., Luong, Q. Nguyen, Peretto, N., Reid, M., Schneider, N., Testi, L., White, G. J., Wilson, C.
We present continuum observations of the Perseus B1-E region from the Herschel Gould Belt Survey. These Herschel data reveal a loose grouping of substructures at 160 - 500 micron not seen in previous submillimetre observations. We measure temperature
Externí odkaz:
http://arxiv.org/abs/1111.7021