منابع مشابه
Local Interstellar Matter: The Apex Cloud
Several nearby individual low column density interstellar cloudlets have been identified previously based on kinematical features evident in high-resolution Ca observations near the Sun. One of these cloudlets, the ‘Apex Cloud” (AC), is within 5 pc of the Sun in the solar apex direction. The question of which interstellar cloud will constitute the next galactic environment of the Sun in princip...
متن کاملLocal Interstellar Matter : The Apex Cloud Priscilla
Several nearby individual low column density interstellar cloudlets have been identified based on kinematical features evident in high-resolution Ca observations near the Sun. One of these cloudlets, the ‘Apex Cloud” (AC), is within 5 pc of the Sun in the solar apex direction. The question of which interstellar cloud will constitute the next galactic environment of the Sun in principle can be d...
متن کاملInterstellar chemistry recorded in organic matter from primitive meteorites.
Organic matter in extraterrestrial materials has isotopic anomalies in hydrogen and nitrogen that suggest an origin in the presolar molecular cloud or perhaps in the protoplanetary disk. Interplanetary dust particles are generally regarded as the most primitive solar system matter available, in part because until recently they exhibited the most extreme isotope anomalies. However, we show that ...
متن کاملAntiprotons from spallations of cosmic rays on interstellar matter
Cosmic ray antiprotons provide an important probe for the study of the galactic Dark Matter, as they could be produced by neutralino annihilations, primordial black holes evaporations or other exotic sources. On the other hand, antiprotons are anyway produced by standard nuclear reactions of cosmic ray nuclei on interstellar matter (spallations), that are known to occur in the Galaxy. This proc...
متن کاملInterstellar Matter and the Boundary Conditions of the Heliosphere
The interstellar cloud surrounding the solar system regulates the galactic environment of the Sun, and determines the boundary conditions of the heliosphere. Both the Sun and interstellar clouds move through space, so these boundary conditions change with time. Data and theoretical models now support densities in the cloud surrounding the solar system of n(H)=0.22±0.06 cm, and n(e)∼0.1 cm, with...
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ژورنال
عنوان ژورنال: Transactions of the International Astronomical Union
سال: 1985
ISSN: 0251-107X
DOI: 10.1017/s0251107x00006532