Zobrazeno 1 - 10
of 314
pro vyhledávání: '"Gutermuth, R."'
Autor:
Nazari, P., Rocha, W. R. M., Rubinstein, A. E., Slavicinska, K., Rachid, M. G., van Dishoeck, E. F., Megeath, S. T., Gutermuth, R., Tyagi, H., Brunken, N., Narang, M., Manoj, P., Watson, D. M., Evans II, N. J., Federman, S., Page, J. Muzerolle, Anglada, G., Beuther, H., Klaassen, P., Looney, L. W., Osorio, M., Stanke, T., Yang, Y. -L.
Publikováno v:
A&A 686, A71 (2024)
Nitrogen-bearing complex organic molecules have been commonly detected in the gas phase but not yet in interstellar ices. This has led to the long-standing question of whether these molecules form in the gas phase or in ices. $\textit{James Webb}$ Sp
Externí odkaz:
http://arxiv.org/abs/2401.07901
Autor:
Balog, Zoltan, Siegler, Nick, Rieke, G. H., Kiss, L. L., Muzerolle, James, Gutermuth, R. A., Bell, Cameron P. M., Vinkó, J., Su, K. Y. L., Young, E. T., Gáspár, András
We present new deep UBVRI images and high-resolution multi-object optical spectroscopy of the young (similar to 6-10 Myr old), relatively nearby (800 pc) open cluster IC 2395. We identify nearly 300 cluster members and use the photometry to estimate
Externí odkaz:
http://hdl.handle.net/10150/622451
http://arizona.openrepository.com/arizona/handle/10150/622451
http://arizona.openrepository.com/arizona/handle/10150/622451
We review the use of young low mass stars and protostars, or young stellar objects (YSOs), as tracers of star formation. Observations of molecular clouds at visible, infrared, radio and X-ray wavelengths can identify and characterize the YSOs populat
Externí odkaz:
http://arxiv.org/abs/2203.03655
We use hydrodynamical simulations of star-forming gas with stellar feedback and sink particles (proxies for young stellar objects, i.e., YSOs) to produce and analyze synthetic 1.1mm continuum observations at different distances (150 - 1000pc) and age
Externí odkaz:
http://arxiv.org/abs/2109.06916
Autor:
Chacon-Tanarro, A., Pineda, J. E., Caselli, P., Bizzocchi, L., Gutermuth, R. A., Mason, B. S., Gomez-Ruiz, A. I., Harju, J., Devlin, M., Dicker, S. R., Mroczkowski, T., Romero, C. E., Sievers, J., Stanchfield, S., Offner, S., Sanchez-Arguelles, D.
Publikováno v:
A&A 623, A118 (2019)
Context: The study of dust emission at millimeter wavelengths is important to shed light on the dust properties and physical structure of pre-stellar cores, the initial conditions in the process of star and planet formation. Aims: Using two new conti
Externí odkaz:
http://arxiv.org/abs/1901.02476
Autor:
Sokol, Alyssa D., Gutermuth, R. A., Pokhrel, R., Gomez-Ruiz, A. I., Wilson, G. W., Offner, S. S. R., Heyer, M., Luna, A., Schloerb, F. P., Sanchez, D.
We present a 1.1~mm census of dense cores in the Mon~R2 Giant Molecular Cloud with the AzTEC instrument on the Large Millimeter Telescope (LMT). We detect 295 cores (209 starless, and 86 with protostars) in a two square degree shallow survey. We also
Externí odkaz:
http://arxiv.org/abs/1811.07024
Autor:
Karnath, N., Prchlik, J. K., Gutermuth, R. A., Allen, T. S., Megeath, S. T., Pipher, J. L., Wolk, S., Jeffries, R. D.
We present a study of the kinematics and structure of the Cep OB3b cluster based on new spectra obtained with the Hectoschelle spectrograph on the MMT and data from Spitzer, Chandr}, and Gaia. At a distance of 819+/-16 pc, Cep OB3b is one of the clos
Externí odkaz:
http://arxiv.org/abs/1811.04505
Autor:
Heyer, M., Wilson, G. W., Gutermuth, R., Lizano, S., Gomez-Ruiz, A., Kurtz, S., Luna, A., Serrano-Bernal, E. O., Schloerb, F. P.
Sensitive, imaging observations of the 1.1 mm dust continuum emission from a 1 deg^2 area collected with the AzTEC bolometer camera on the Large Millimeter Telescope are presented. A catalog of 1545 compact sources is constructed based on a Wiener-op
Externí odkaz:
http://arxiv.org/abs/1709.09059
Filamentary structures are ubiquitous in molecular clouds, and have been recently argued to play an important role in regulating the size and mass of embedded clumps through fragmentation and mass accretion. Here, we reveal the dynamical state and fr
Externí odkaz:
http://arxiv.org/abs/1610.10066
Autor:
Pokhrel, R., Gutermuth, R., Ali, B., Megeath, T., Pipher, J., Myers, P., Fischer, W. J., Henning, T., Wolk, S. J., Allen, L., Tobin, J. J.
We present a far-IR survey of the entire Mon R2 GMC with $Herschel-SPIRE$ cross-calibrated with $Planck-HFI$ data. We fit the SEDs of each pixel with a greybody function and an optimal beta value of 1.8. We find that mid-range column densities obtain
Externí odkaz:
http://arxiv.org/abs/1606.01752