HH 1/2
J2000.0 epoch | |
---|---|
Right ascension | 05h 36m 22.8s[1] |
Declination | −06° 46′ 03″[1] |
Distance | 1500[2] ly |
Constellation | Orion[2] |
Designations | HH 1-2, HH 1/2, HH 1, HH 2 |
The
km/s.[2]
The central region
The central region contains an opaque cloud core with an
Microns. These sources were first detected with the Very Large Array and are therefore named VLA 1 and 2.[9] The source HH 1-2 VLA 1[10] drives the HH 1/2 pair and the source VLA 2 drives the Herbig-Haro objects HH 144/145.[11] There might be even a third outflow in the central region of HH 1/2, indicating a third member.[12]
The jet towards HH 1 is visible in optical images, but the counterjet towards HH 2 was detected in the infrared with the Spitzer Space Telescope.[13]
Gallery
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An older version of the region mapped by the WFPC2 of the Hubble Space Telescope. The image also shows the jet in the lower right part in more detail
-
Multiple Herbig-Haro Objects mapped by the Hubble Space Telescope, including HH 2 at the lower right.HH 47 is at the top part and part of HH 34is at the lower left.
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The reflection nebula NGC 1999 (blue cloud in the center) and the Herbig-Haro Objects HH 1/2 below NGC 1999 as small pink clouds.
References
- ^ a b "HH 1-2". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-02-15.
- ^ S2CID 118242041.
- ^ ISSN 0004-637X.
- ISSN 0004-637X.
- S2CID 125612968.
- ISSN 0004-6256.
- S2CID 13878953.
- ISSN 0185-1101.
- S2CID 59520064.
- ^ "HH 1-2 VLA 1". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-02-15.
- ISSN 0004-637X.
- ISSN 0004-6256.
- S2CID 1793062.