HH 24-26
HH 24-26 is a molecular cloud and star-forming region containing the Herbig-Haro objects HH 24, HH 25 and HH 26. This region contains the highest concentration of astrophysical jets known anywhere in the sky. The molecular cloud is located about 1400 light-years away in the L1630 dark cloud, which is part of the Orion B molecular cloud in the constellation of Orion.

The region contains multiple protostars (two class 0 and one class I) and four more evolved IRAS sources. The three protostars are driving the Herbig-Haro objects in this region.
Q272447
molecular cloud
Concept
Q16744
star-forming region
Concept
Q50048
Herbig-Haro objects
Concept
Q284657
astrophysical jet
Concept
Q531
light-year
Concept
Q204194
dark cloud
Concept
Q16742
Orion B molecular cloud
CEL
Q8860
Orion
Concept
Q204903
protostar
Concept
Q724913
IRAS
MISC
Q87120860
HH 24-26
UNK
1400-01-01T00:00:00Z^^http://www.w3.org/2001/XMLSchema#dateTime
1400
DATE
+24^^http://www.w3.org/2001/XMLSchema#decimal
24
NUMBER
-26^^http://www.w3.org/2001/XMLSchema#decimal
-26
NUMBER
+24^^http://www.w3.org/2001/XMLSchema#decimal
24
NUMBER
+25^^http://www.w3.org/2001/XMLSchema#decimal
25
NUMBER
+26^^http://www.w3.org/2001/XMLSchema#decimal
26
NUMBER
+1630^^http://www.w3.org/2001/XMLSchema#decimal
1630
NUMBER
0^^http://www.w3.org/2001/XMLSchema#decimal
0
NUMBER
part of
named after