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Μεσοαστρική Ύλη

H 2. Η. Αέριο (99%). HI (21 cm). ΗΙΙ (H α emission, συνεχές στα ραδιοκύματα και υπέρυθρο). Μεσοαστρική Ύλη. He. Σκόνη (1%). Κοσμική Ακτινοβολία. Μαγνητικό πεδίο ( ≈ 3 μ G ). Μεσοαστρική Ύλη.

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Μεσοαστρική Ύλη

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  1. H2 Η Αέριο (99%) HI (21 cm) ΗΙΙ (Hα emission, συνεχές στα ραδιοκύματα και υπέρυθρο) Μεσοαστρική Ύλη He Σκόνη (1%) Κοσμική Ακτινοβολία Μαγνητικό πεδίο (≈ 3 μG)

  2. Μεσοαστρική Ύλη

  3. The spiral galaxy M 81: a colour-coded composite of radio observations of atomic hydrogen (blue) made with the Very Large Array (VLA) and infrared observations made with the SPITZER Space Telescope (green and red). Scientists at MPIA use data like these to study the influence of the large-scale distribution of interstellar matter on the star formation process.

  4. Μεσοαστρική σκόνη Σύνθεση: Άνθρακας Σίδηρος Πυρίτιο Μαγνήσιο Θείο Αργίλιο Άζωτο

  5. Μεσοαστρικό Αέριο

  6. ΗΙΙ Περιοχές – Ο, Β αστέρες

  7. ΗΙΙ - Πλανητικά Νεφελώματα

  8. ΗΙΙ - Κελύφη υπερκαινοφανών

  9. Ανακύκλωση στο Μεσοαστρικό Χώρο

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