Amenable
发表于 2025-3-25 06:09:06
Saskia Bruysten,Henning Engelkeown asteroids were also observed. There is an apparent difference in the albedo distribution of the asteroids as a function of size, however, this effect is probably an artifact due to a combination of factors such as faint source flux overestimation and confusion with faint background sources.
Bernstein-test
发表于 2025-3-25 08:27:32
http://reply.papertrans.cn/24/2302/230146/230146_22.png
Deadpan
发表于 2025-3-25 13:45:58
http://reply.papertrans.cn/24/2302/230146/230146_23.png
GIST
发表于 2025-3-25 19:22:54
Christian Seelos,Kate Ganly,Johanna Mairsults about temperature T, global volume intensity ℜ, albedo of the dust ., and their gradients with heliocentric distance r (in AU) are derived in the ecliptic from the available IRAS observations. Typically T is found to be of the order of 250 r. K and . of the order of 0.09 r..
画布
发表于 2025-3-25 22:15:50
Anne Clifford,Sarah E. A. Dixond based telescopes observations carried out by both amature and professional astronomers. In this overview we will discuss only the part of the data set that is of most interest ot infrared astromers, namely the nucleus and the dust. The molecular emission has been dealt with in another chapter.
Metamorphosis
发表于 2025-3-26 02:40:49
http://reply.papertrans.cn/24/2302/230146/230146_26.png
推延
发表于 2025-3-26 08:16:13
A Review of Social Entrepreneurship Researchcm and 6cm radio continuum surveys made with the same angular resolution. As well as indicating that the 60 .m emission from this region comes in a large part from dust associated with the extended low density . regions, this provides a way of separating the thermal and synchrotron components of the radio emission.
STELL
发表于 2025-3-26 09:50:28
The Challenge of Public Goods Provisionhe origin of the infrared emission from the solar neigbourhood. We show that altough most of the emission comes from interstellar matter not associated with current star formation, about half of the heating of grains is provided by ultraviolet photons radiated by stars younger than few 10. yrs.
毁坏
发表于 2025-3-26 16:39:27
Individual Incentive Strategiesrstellar medium (HI, H., and HII) in cirrus, reflection nebulae, and HII regions. Taking into account the various constraints on the different dust components, in particular coming from IRAS data, we show that a bimodal rather than continuous size distribution between small and big grains is the most favorable solution.
colostrum
发表于 2025-3-26 20:41:08
The Resource Dependency of Organizationsof the surrounding regions. The dominant dust heating mechanism appears to be ultraviolet radiation, either from stellar wind shooks or direct stellar radiation from hotter stars. The infrared luminosities from these extended emitting regions are often an appreciable fraction of that of the central star.