Zobrazeno 1 - 10
of 32
pro vyhledávání: '"Knez, Claudia"'
Autor:
Staguhn, Johannes, Mandell, Avi, Stevenson, Kevin, Saxena, Prabal, Kopparapu, Ravi, Fixsen, Dale, Sharp, Elmer, DiPirro, Michael, Knez, Claudia, Wolf, Eric, Sotzen, Kristin, Mandt, Kathleen, Gong, Qian, Villanueva, Geronimo
This White Paper presents a mission concept called MIRECLE - the Mid-InfraRed Exoplanet CLimate Explorer. With a moderately sized aperture of 2 meters, broad wavelength coverage (4 - 25 um), and next generation instruments, MIRECLE will be capable of
Externí odkaz:
http://arxiv.org/abs/1908.02356
Autor:
Peterson, Dawn E., Garatti, Alessio Caratti o, Bourke, Tyler L., Forbrich, Jan, Gutermuth, Robert A., Jorgensen, Jes K., Allen, Lori E., Patten, Brian M., Dunham, Michael M., Harvey, Paul M., Merin, Bruno, Chapman, Nicholas L., Cieza, Lucas A., Huard, Tracy L., Knez, Claudia, Prager, Brian, Evans II, Neal J.
We present Spitzer Space Telescope IRAC and MIPS observations of a 0.85 deg^2 field including the Corona Australis (CrA) star-forming region. At a distance of 130 pc, CrA is one of the closest regions known to be actively forming stars, particularly
Externí odkaz:
http://arxiv.org/abs/1104.1669
We have mapped over 50 massive, dense clumps with four dense gas tracers: HCN J=1-0 and 3-2; and CS J=2-1 and 7-6 transitions. Spectral lines of optically thin H^{13}CN 3-2 and C^{34}S 5-4 were also obtained towards the map centers. These maps usuall
Externí odkaz:
http://arxiv.org/abs/1004.0398
We have mapped 63 regions forming high-mass stars in CS J=5-4 using the CSO. The CS peak position was observed in C34S J=5-4 towards 57 cores and in 13CS J=5-4 towards the 9 brightest cores. The sample is a subset of a sample originally selected towa
Externí odkaz:
http://arxiv.org/abs/astro-ph/0308310
Our knowledge of the initial conditions and early stages of high mass star formation is very limited. We will review recent surveys of regions in the early stages of massive star formation using molecular tracers of high density and dust continuum em
Externí odkaz:
http://arxiv.org/abs/astro-ph/0111103
In this survey we have systematically mapped 63 cloud cores in the CS J = 5 -> 4 line towards a sample of high mass star forming cores with water masers (Plume et al. 1992, Plume et al. 1997) using the CSO. From the CS spectra and maps we determine c
Externí odkaz:
http://arxiv.org/abs/astro-ph/0111100
Twenty-four cores have been mapped in CS J = 7 -> 6 at the CSO. From the spectra we determine core sizes and virial masses. Combining results from the CS and dust continuum studies for M8E, we use Monte Carlo simulations for the CS emission to determ
Externí odkaz:
http://arxiv.org/abs/astro-ph/0111105
Autor:
Greathouse, Thomas K., Lacy, John H., Bézard, Bruno, Moses, Julianne I., Richter, Matthew J., Knez, Claudia
Publikováno v:
In Icarus 2006 181(1):266-271
Publikováno v:
2016 IEEE Aerospace Conference; 2016, p1-8, 8p