Zobrazeno 1 - 10
of 148
pro vyhledávání: '"Kulesa, C. A."'
Autor:
Saldaño, H. P., Rubio, M., Bolatto, A. D., Sandstrom, K., Swift, B. J., Verdugo, C., Jameson, K., Walker, C. K., Kulesa, C., Spilker, J., Bergman, P., Salazar, G. A.
Publikováno v:
A&A 687, A26 (2024)
We present the CO(3-2) APEX survey at 6 pc resolution of the bar of the SMC. We aboard the CO analysis in the SMC-Bar comparing the CO(3-2) survey with that of the CO(2-1) of similar resolution. We study the CO(3-2)-to-CO(2-1) ratio (R32) that is ver
Externí odkaz:
http://arxiv.org/abs/2311.00145
Autor:
Stanke, Thomas, Arce, H. G., Bally, J., Bergman, P., Carpenter, J., Davis, C. J., Dent, W., Di Francesco, J., Eislöffel, J., Froebrich, D., Ginsburg, A., Heyer, M., Johnstone, D., Mardones, D., McCaughrean, M. J., Megeath, S. T., Nakamura, F., Smith, M. D., Stutz, A., Tatematsu, K., Walker, C., Williams, J. P., Zinnecker, H., Swift, B. J., Kulesa, C., Peters, B., Duffy, B., Kloosterman, J., Yıldız, U. A., Pineda, J. L., De Breuck, C., Klein, Th.
Publikováno v:
A&A 658, A178 (2022)
The Orion molecular cloud complex harbours the nearest GMCs and site of high-mass star formation. Its YSO populations are thoroughly characterized. The region is therefore a prime target for the study of star formation. Here, we verify the performanc
Externí odkaz:
http://arxiv.org/abs/2201.00463
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Zmuidzinas, Jonas, Gao, Jian-Rong, Silva, J. R. G., Laauwen, W. M., Mirzaei, B., Vercruyssen, N., Finkel, M., Westerveld, M., More, N., Silva, V., Young, A., Kulesa, C., Walker, C., van der Tak, F., Gao, J. R.
Publikováno v:
Proceedings of SPIE; August 2024, Vol. 13102 Issue: 1 p131020I-131020I-14, 12970995p
Autor:
Monelli, M., Testa, V., Bono, G., Ferraro, I., Iannicola, G., Fiorentino, G., Arcidiacono, C., Massari, D., Boutsia, K., Briguglio, R., Busoni, L., Carini, R., Close, L., Cresci, G., Esposito, S., Fini, L., Fumana, M., Guerra, J. C., Hill, J., Kulesa, C., Mannucci, F., McCarthy, D., Pinna, E., Puglisi, A., Quiros-Pacheco, F., Ragazzoni, R., Riccardi, A., Skemer, A., Xompero, M.
We present deep near-infrared (NIR) J, Ks photometry of the old, metal-poor Galactic globular cluster M\,15 obtained with images collected with the LUCI1 and PISCES cameras available at the Large Binocular Telescope (LBT). We show how the use of Firs
Externí odkaz:
http://arxiv.org/abs/1507.08845
The M-dwarfs in Multiples (MinMs) survey - I. Stellar multiplicity among low-mass stars within 15 pc
Autor:
Ward-Duong, K., Patience, J., De Rosa, R. J., Bulger, J., Rajan, A., Goodwin, S. P., Parker, Richard J., McCarthy, D. W., Kulesa, C.
We present a large-scale, volume-limited companion survey of 245 late-K to mid-M (K7-M6) dwarfs within 15 pc. Infrared adaptive optics (AO) data were analysed from the Very Large Telescope, Subaru Telescope, Canada-France-Hawaii Telescope, and MMT Ob
Externí odkaz:
http://arxiv.org/abs/1503.00724
Autor:
De Rosa, R. J., Patience, J., Ward-Duong, K., Vigan, A., Marois, C., Song, I., Macintosh, B., Graham, J. R., Doyon, R., Bessell, M. S., Lai, O., McCarthy, D. W., Kulesa, C.
We report the discovery of a wide co-moving substellar companion to the nearby ($D=67.5\pm1.1$ pc) A3V star $\zeta$ Delphini based on imaging and follow-up spectroscopic observations obtained during the course of our Volume-limited A-Star (VAST) mult
Externí odkaz:
http://arxiv.org/abs/1410.0005
We mapped 12CO and 13CO J = 2-1 emission over 1.04 square deg of the Serpens molecular cloud with 38 arcsec spatial and 0.3 km/s spectral resolution using the Arizona Radio Observatory Heinrich Hertz Submillimeter telescope. Our maps resolve kinemati
Externí odkaz:
http://arxiv.org/abs/1311.4028
Autor:
Bulger, J., Hufford, T., Schneider, A., Patience, J., Song, I., De Rosa, R. J., Rajan, A., Dowell, C. D., McCarthy, D., Kulesa, C.
A set of six debris disk candidates identified with IRAS or WISE excesses were observed at either 350 um or 450 um with the CSO. Five of the targets - HIP 51658, HIP 68160, HIP 73512, HIP 76375, and HIP 112460 - have among the largest measured excess
Externí odkaz:
http://arxiv.org/abs/1307.4015
Autor:
Esposito, S., Mesa, D., Skemer, A., Arcidiacono, C., Claudi, R. U., Desidera, S., Gratton, R., Mannucci, F., Marzari, F., Masciadri, E., Close, L., Hinz, P., Kulesa, C., McCarthy, D., Males, J., Agapito, G., Argomedo, J., Boutsia, K., Briguglio, R., Brusa, G., Busoni, L., Cresci, G., Fini, L., Fontana, A., Guerra, J. C., Hill, J. M., Miller, D., Paris, D., Pinna, E., Puglisi, A., Quiros-Pacheco, F., Riccardi, A., Stefanini, P., Testa, V., Xompero, M., Woodward, C.
We have performed H and Ks band observations of the planetary system around HR 8799 using the new AO system at the Large Binocular Telescope and the PISCES Camera. The excellent instrument performance (Strehl ratios up to 80% in H band) enabled detec
Externí odkaz:
http://arxiv.org/abs/1203.2735