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Table D.1
Detailed descriptions of the sub-regions where MHOs (see Table A.1) were identified.
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Area including MHO 900. Despite the overall resemblance to an edge-on disk system with a bipolar outflow cavity we were unable to identify any IRAS or AKARI sources here. The system is most likely a broken bow-shock driven from V2494 Cyg. |
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Area including the MHO 901 complex coinciding with the optical HH 382G, F and E knots. |
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Area including the MHO 902 knots which coincide with the optical HH 382A, B and C knots. |
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This sub field includes MHO 903 which is rather diffuse in structure. |
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The area shows the MHO 904 knots which belong to the outflow emanated from V2494 Cyg. These are the most southern knots discovered in our survey. |
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MHO 905 is a small bow-shock, the origin of which is still unknown. |
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This is one of the knots in the MHO 906 outflow. This feature is associated with HH 380F. |
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Part of the MHO 906 outflow coinciding with HH 380B. |
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Last part of the MHO 906 outflow coinciding with the optical feature HH 380C. Morphologically it resembles a bow-shock driven from the southeast. In this current work we assume an outflow direction to the southwest. |
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Area includes the MHO 907 complex bow shock which coincides with the faint object HH 970. IRAS 20575+5218 is unrelated to this flow. |
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Region including the MHO 908 chain of knots A to D, where knot D might be related to HH 974B. The IRAS 20575+5210 error ellipse and CN4 are marked for reference. |
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Area shows a chain of relatively faint knots comprising MHO 909. |
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Area shows the details of MHO 910, which is associated with the prominent optical bow-shock HH 380(A). There is a faint extension to the east-northeast (MHO 910B) which could be unrelated to this flow. MHO 910C also coincides with HH 380E. |
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Region where the MHO 911 bow-shock can be seen. This quite prominent and compact bow also coincides with HH 627A. |
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Figure shows the complex bow-shock structure MHO 912, which is part of a prominent bipolar outflow that is only detected in the near-infrared. |
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Area including the compact bipolar outflow MHO 913, emanating from IRAS 20583+5228. Knots A and B correspond to HH 975A and B. |
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Figure shows the complex bow-shock structure of MHO 914. |
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Area including the MHO 915 chain of knots emanating from Cyg 19. These are part of a prominent near-infrared bipolar outflow. |
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Region including the faint knot MHO 916 which coincides with HH 629 and emanates from V2495 Cyg. |
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The compact knot MHO 917 coinciding with HH 670. |
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The faint diffuse bow-shock MHO 918. |
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MHO 919 knots also coinciding with the HH 631 knots D and E. |
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Area including MHO 920 and 921 which is also full of HH objects, some coinciding with the near-infrared features. The IRAS 20588+5215 (IRAS 15) error ellipse is shown, as is the position of CN2. |
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Area including the extensive and rather complex chain of bow-shocks MHO 922, which is part of a near-infrared bipolar outflow. |
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Region showing the complex object MHO 923, which coincides with HH 448 and is also known as RNO 127. MHO 926A, which coincides with HH 634A, can also be seen in this image. |
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Area shows the MHO 924 bright knot which coincides with HH 635A. |
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Area shows MHO 925 which coincides with HH 633. |
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Area shows the MHO 926 outflow, which also coincides with the optical HH 634 outflow. |
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Region shows the MHO 927 group of knots and bow-shocks which coincide with HH 635B and C. This is part of the flow driven by V2495 Cyg. |
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Group of bows and knots emanating from IRAS 21005+5217. MHO 928 and 929 are thought to be the part of a west-to-east or east-to-south bipolar flow. MHO 930 is part of a bipolar outflow extending in a SW-NE direction. |
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Area including MHO 932 and 931. These two objects are thought to belong to different flows. |
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Region shows the MHO 933 knots which are thought to be driven by IRAS 21005+5217. MHO 933 belongs to the same bipolar outflow as MHO 928 and 929. |
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The area shows the MHO 934 chain of bow-shocks which are thought to be driven by a source somewhere in the SE. |
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Region shows MHO 935 which is driven by IRAS 21005+5217. MHO 935 belongs to the same bipolar outflow as MHO 930. |
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Area shows MHO 936 which has quite a complex structure. It is thought to be driven by a source somewhere in the northeast. |
In each case images are presented in H2 1−0 S(1) line emission before (left) and after (right) continuum subtraction. The positions of known Herbig-Haro (HH) objects, cometary nebulae (CN) and IRAS sources are indicated.
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