2019-12-16 20:00:49
Explanation: Can magnetic fields help tell us how spiral galaxies form and evolve? To find out, the HAWC+ instrument on NASA's airborne (747) SOFIA observatory observed nearby spiral galaxy M77. HAWC+ maps magnetism by observing polarized infrared light emitted by elongated dust grains rotating in alignment with the local magnetic field.
The HAWC+ image shows that magnetic fields do appear to trace the spiral arms in the inner regions of M77, arms that likely highlight density waves in the inflowing gas, dust and stars caused by the gravity of the galaxy's oval shape.
The featured picture superposes the HAWC+ image over diffuse X-ray emission mapped by NASA's NuSTAR satellite and visible light images taken by Hubble and the SDSS. M77 is located about 47 million light years away toward the constellation of the Sea Monster (Cetus).
via
olalathos
The HAWC+ image shows that magnetic fields do appear to trace the spiral arms in the inner regions of M77, arms that likely highlight density waves in the inflowing gas, dust and stars caused by the gravity of the galaxy's oval shape.
The featured picture superposes the HAWC+ image over diffuse X-ray emission mapped by NASA's NuSTAR satellite and visible light images taken by Hubble and the SDSS. M77 is located about 47 million light years away toward the constellation of the Sea Monster (Cetus).
via
olalathos
ΜΟΙΡΑΣΤΕΙΤΕ
ΔΕΙΤΕ ΑΚΟΜΑ
ΠΡΟΗΓΟΥΜΕΝΟ ΑΡΘΡΟ
Σοκ: 15.000 οι αποποιήσεις κληρονομιάς το α' 4μηνο του 2019
ΕΠΟΜΕΝΟ ΑΡΘΡΟ
Παιδικά βιβλία φυσικής για όλους
ΣΧΟΛΙΑΣΤΕ
