Celestial hemisphere:  Northern  ·  Constellation: Taurus (Tau)
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Barnard 207 / LDN 1489 / LDN 1491 / LBN 777, Prodromos
Barnard 207 / LDN 1489 / LDN 1491 / LBN 777
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Barnard 207 / LDN 1489 / LDN 1491 / LBN 777

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Barnard 207 / LDN 1489 / LDN 1491 / LBN 777, Prodromos
Barnard 207 / LDN 1489 / LDN 1491 / LBN 777
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Barnard 207 / LDN 1489 / LDN 1491 / LBN 777

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Description

Barnard 207, LDN 1489, LDN 1491, and LBN 777 are regions within the interstellar medium characterized by significant dust concentrations. These dark nebulae exhibit high levels of obscuration, causing them to appear as opaque clouds against the backdrop of celestial objects. The dust present in these regions consists of micron-sized particles composed primarily of carbonaceous and silicate materials. These dark nebulae are sites of interest for astrophysical studies, as the obscuring dust plays a crucial role in the formation and evolution of stars and planetary systems. Observations of these regions in various wavelengths, from infrared to radio, provide insights into the complex interplay between interstellar matter and the processes shaping the cosmos.

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Barnard 207 / LDN 1489 / LDN 1491 / LBN 777, Prodromos

In these public groups

S.P.I.C.A. Cyprus Remote Observatory