Zobrazeno 1 - 10
of 81
pro vyhledávání: '"Sánchez-Gallego J"'
Autor:
Kreckel, K., Egorov, O. V., Egorova, E., Blanc, G. A., Drory, N., Kounkel, M., Mendez-Delgado, J. E., Roman-Zuniga, C. G., Sanchez, S. F., Stringfellow, G. S., Stutz, A. M., Zari, E., Barrera-Ballesteros, J. K., Bizyaev, D., Brownstein, J. R., Congiu, E., Fernandez-Trincado, J. G., Garcia, P., Hillenbrand, L., Ibarra-Medel, H. J., Jin, Y., Johnston, E. J., Jones, A. M., Kim, J. Serena, Kollmeier, J. A., Kong, S., Krishnarao, D., Kumari, N., Li, J., Long, K., Mata-Sanchez, A., Mejia-Narvaez, A., Popa, S. A., Rix, H-W, Sattler, N., Serna, J., Singh, A., Sanchez-Gallego, J. R., Wofford, A., Wong, T.
Publikováno v:
A&A 689, A352 (2024)
The Orion Molecular Cloud complex, one of the nearest (D = 406 pc) and most extensively studied massive star-forming regions, is ideal for constraining the physics of stellar feedback, but its ~12 deg diameter on the sky requires a dedicated approach
Externí odkaz:
http://arxiv.org/abs/2405.14943
Autor:
Wilson, J. C., Hearty, F. R., Skrutskie, M. F., Majewski, S. R., Holtzman, J. A., Eisenstein, D., Gunn, J., Blank, B., Henderson, C., Smee, S., Nelson, M., Nidever, D., Arns, J., Barkhouser, R., Barr, J., Beland, S., Bershady, M. A., Blanton, M. R., Brunner, S., Burton, A., Carey, L., Carr, M., Colque, J. P., Crane, J., Damke, G. J., Davidson Jr., J. W., Dean, J., Di Mille, F., Don, K. W., Ebelke, G., Evans, M., Fitzgerald, G., Gillespie, B., Hall, M., Harding, A., Harding, P., Hammond, R., Hancock, D., Harrison, C., Hope, S., Horne, T., Karakla, J., Lam, C., Leger, F., MacDonald, N., Maseman, P., Matsunari, J., Melton, S., Mitcheltree, T., O'Brien, T., O'Connell, R. W., Patten, A., Richardson, W., Rieke, G., Rieke, M., Roman-Lopes, A., Schiavon, R. P., Sobeck, J. S., Stolberg, T., Stoll, R., Tembe, M., Trujillo, J. D., Uomoto, A., Vernieri, M., Walker, E., Weinberg, D. H., Young, E., Anthony-Brumfield, B., Bizyaev, D., Breslauer, B., De Lee, N., Downey, J., Halverson, S., Huehnerhoff, J., Klaene, M., Leon, E., Long, D., Mahadevan, S., Malanushenko, E., Nguyen, D. C., Owen, R., Sanchez-Gallego, J. R., Sayres, C., Shane, N., Shectman, S. A., Shetrone, M., Skinner, D., Stauffer, F., Zhao, B.
We describe the design and performance of the near-infrared (1.51--1.70 micron), fiber-fed, multi-object (300 fibers), high resolution (R = lambda/delta lambda ~ 22,500) spectrograph built for the Apache Point Observatory Galactic Evolution Experimen
Externí odkaz:
http://arxiv.org/abs/1902.00928
We present an analysis of the radial profiles of a sample of 43 HI-flux selected spiral galaxies from the Nearby Galaxies Legacy Survey (NGLS) with resolved James Clerk Maxwell Telescope (JCMT) CO $J=3-2$ and/or Very Large Array (VLA) HI maps. Compar
Externí odkaz:
http://arxiv.org/abs/1702.02118
Autor:
Mok, Angus, Wilson, C. D., Golding, J., Warren, B. E., Israel, F. P., Serjeant, S., Knapen, J. H., Sanchez-Gallego, J. R., Barmby, P., Bendo, G. J., Rosolowsky, E., van der Werf, P.
We present a study of the molecular gas properties in a sample of 98 HI - flux selected spiral galaxies within $\sim25$ Mpc, using the CO $J=3-2$ line observed with the James Clerk Maxwell Telescope. We use the technique of survival analysis to incor
Externí odkaz:
http://arxiv.org/abs/1512.05768
Autor:
Tan, Boon-Kok, Leech, J., Rigopoulou, D., Warren, B. E., Wilson, C. D., Attewell, D., Azimlu, M., Bendo, G. J., Butner, H. M., Brinks, E., Chanial, P., Clements, D. L., Heesen, V., Israel, F., Knapen, J. H., Matthews, H. E., Mortier, A. M. J., Mühle, Sánchez-Gallego, J. R., Tilanus, R. P. J., Usero, A., van der Werf, P., Zhu, M.
We present $^{12}$CO \textit{J=3$\rightarrow$2} maps of NGC 2976 and NGC 3351 obtained with the James Clerk Maxwell Telescope (JCMT), both early targets of the JCMT Nearby Galaxy Legacy Survey (NGLS). We combine the present observations with $^{12}$C
Externí odkaz:
http://arxiv.org/abs/1308.6209
Using a simple model of photodissociated atomic hydrogen on a galactic scale, it is possible to derive total hydrogen volume densities. These densities, obtained through a combination of atomic hydrogen, far-ultraviolet and metallicity data, provide
Externí odkaz:
http://arxiv.org/abs/1210.6409
Autor:
Wilson, C. D., Warren, B. E., Israel, F. P., Serjeant, S., Attewell, D., Bendo, G. J., Butner, H. M., Chanial, P., Clements, D. L., Golding, J., Heesen, V., Irwin, J., Leech, J., Matthews, H. E., Muhle, S., Mortier, A. M. J., Petitpas, G., Sanchez-Gallego, J. R., Sinukoff, E., Shorten, K., Tan, B. K., Tilanus, R. P. J., Usero, A., Vaccari, M., Wiegert, T., Zhu, M., Alexander, D. M., Alexander, P., Azimlu, M., Barmby, P., Borys, C., Brar, R., Bridge, C., Brinks, E., Brooks, S., Coppin, K., Cote, S., Cote, P., Courteau, S., Davies, J., Eales, S., Fich, M., Hudson, M., Hughes, D. H., Ivison, R. J., Knapen, J. H., Page, M., Parkin, T. J., Pope, A., Rigopoulou, D., Rosolowsky, E., Seaquist, E. R., Spekkens, K., Tanvir, N., van der Hulst, J. M., van der Werf, P., Vlahakis, C., Webb, T. M., Weferling, B., White, G. J.
The James Clerk Maxwell Telescope Nearby Galaxies Legacy Survey (NGLS) comprises an HI-selected sample of 155 galaxies spanning all morphological types with distances less than 25 Mpc. We describe the scientific goals of the survey, the sample select
Externí odkaz:
http://arxiv.org/abs/1206.1629
We present H\alpha{} fluxes, star formation rates (SFRs) and equivalent widths (EWs) for a sample of 156 nearby galaxies observed in the 12CO J=3-2 line as part of the James Clerk Maxwell Telescope Nearby Galaxies Legacy Survey. These are derived fro
Externí odkaz:
http://arxiv.org/abs/1203.0001
Autor:
Sánchez-Gallego, J. R., Knapen, J. H., Heiner, J. S., Wilson, C. D., Warren, B. E., Allen, R. J., Azimlu, M., Barmby, P., Bendo, G. J., Comerón, S., Israel, F. P., Serjeant, S., Tilanus, R. P. J., Vlahakis, C., van der Werf, P.
We present a first complete 12 CO J=3-2 map of M81, observed as part of the Nearby Galaxies Legacy Survey being carried out at the James Clerk Maxwell Telescope. We detect 9 regions of significant CO emission located at different positions within the
Externí odkaz:
http://arxiv.org/abs/1011.5116
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.