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Table A.15:

A list of all known MHOs in Cassiopeia and Chamaeleon.

Objecta 		RAa Deca Other IDb HHc Referencesd Comment Region
MHO 2900 00 44 56.6 +55 46 53 ${\rm [VDR] 1-1}$ - 71 Faint feature $\sim $30 $^{\prime\prime}$ south of IRAS 00420+5530 Cassiopeia
MHO 2901 00 44 57.6 +55 46 56 ${\rm [VDR] 1-2}$ - 71 Faint feature $\sim $30 $^{\prime\prime}$ south of IRAS 00420+5530 Cassiopeia
MHO 2902 00 44 58.9 +55 47 11 ${\rm [VDR] 1-3}$ - 71 Faint line emission southeast of IRAS 00420+5530 Cassiopeia
MHO 2903 00 45 01.3 +55 47 36 ${\rm [VDR] 1-4}$ - 71 Faint object $\sim $40 $^{\prime\prime}$ northeast of IRAS 00420+5530 Cassiopeia
MHO 2904 00 21 00.7 +62 39 38 ${\rm - }$ - 26 Two faint southward-facing bow shocks near IRAS 00182+6223 Cassiopeia
MHO 2907 00 28 42.2 +56 41 57 ${\rm CB3 k1-k4}$ - 164 North-south chain of 4 knots in globule CB3 Cassiopeia
MHO 2908 03 27 34.5 +58 47 00 ${\rm - }$ - 80 Collimated jet extending N-S over $\sim $2$^\prime$ in the AFGL 490 region Cassiopeia
MHO 2909 03 27 34.8 +58 46 20 ${\rm A}$ - 80 Bright, elongated knot $\sim $1$^\prime$ southwest of AFGL 490 IRS Cassiopeia
MHO 2910 01 23 18.3 +61 48 12 ${\rm S187:SCP 1}$ - 173 Remarkable curving arc of knots and emission in the S187 region Cassiopeia
MHO 2911 01 23 22.0 +61 48 54 ${\rm S187:SCP 2}$ - 173 Small group of knots $\sim $30 $^{\prime\prime}$ northwest of IRAS 01202+6133 in S187 Cassiopeia
MHO 2912 01 23 31.7 +61 47 35 ${\rm S187:SCP 3}$ - 173 Elongated feature $\sim $1.5$^\prime$ south of IRAS 01202+6133 in S187 Cassiopeia
MHO 2913 01 23 35.7 +61 47 37 ${\rm S187:SCP 4}$ - 173 Bow shaped feature next to MHO 2912 in S187 Cassiopeia
MHO 2914 01 23 31.0 +61 50 25 ${\rm S187:SCP 5}$ - 173 Group of knots $\sim $1.5$^\prime$ north of IRAS 01202+6133 in S187 Cassiopeia
               
MHO 3000 12 55 50.3 -76 56 23 ${\rm - }$ HH 54 8, 17, 174, 40, 175 Group of bright knots, arcs and filaments Chameleon
MHO 3001 11 09 22.4 -76 33 33 ${\rm A}$ - 176 Faint feature in western outflow lobe from ISO-ChaI 192 Chameleon
MHO 3002 11 09 22.5 -76 34 34 ${\rm B1, B2}$ - 176 Two knots on either side of T Tauri star C1-6 Chameleon
MHO 3003 11 09 48.9 -76 33 59 ${\rm C1-C3 }$ - 176 Knotty bow shock in eastern outflow lobe from ISO-ChaI 192 Chameleon
MHO 3004 11 09 49.6 -76 34 38 ${\rm D}$ - 176 Faint arc, possibly part of eastern ISO-ChaI 192 flow lobe and/or MHO 3003 Chameleon
MHO 3005 12 55 15.5 -76 57 30 ${\rm - }$ HH 53 177 Group of knots and filaments $\sim $1.5$^\prime$ southwest of MHO 3000/HH 54 Chameleon
MHO 3006 12 55 07.5 -76 57 55 ${\rm - }$ HH 52 177 Group of knots $\sim $2.0$^\prime$ southwest of MHO 3000/HH 54 Chameleon

Notes. (a) Catalogue reference for the Molecular Hydrogen emission-line Object (MHO), with coordinates. (b) Other identification used in the literature. (c) Associated Herbig-Haro object, if any. (d) References to papers presenting near-IR images (including papers citing other IDs): 1. Stanke et al. (2002), 2. Davis et al. (2009), 3. Yu et al. (1997), 4. Yu et al. (2000), 5. Stanke et al. (1998), 6. Gålfalk & Olofsson (2007a), 7. Gålfalk & Olofsson (2008), 8. Zealey et al. (1993), 9. Reipurth et al. (2000b), 10. Davis et al. (2000a), 11. Zealey et al. (1992), 12. Davis et al. (1994b), 13. Davis et al. (2000b), 14. Noriega-Crespo et al. (1994), 15. Noriega-Crespo et al. (1997), 16. Reipurth et al. (2000a), 17. Gredel (1994), 18. Schwartz & Greene (1999), 19. Schwartz, Greene (2003), 20. Davis & Eislöffel (1995), 21. Schwartz et al. (1997), 22. Chrysostomou et al. (2000), 23. Hodapp & Ladd (1995), 24. Davis et al. (1997), 25. O'Connell et al. (2004), 26. Connelley et al. (2007), 27. Garden et al. (1990), 28. Eisloeffel (1999), 29. Davis et al. (1994c), 30. Noriega-Crespo et al. (1996) 31. Garnavich et al. (1997) 32. Gredel & Reipurth (1993), 33. Gredel & Reipurth (1994), 34. Reipurth et al. (1997), 35. Reipurth et al. (1999), 36. Coppin et al. (1998), 37. Bontemps et al. (1996), 38. Davis et al. (2002), 39. Wang et al. (2005), 40. Caratti o Garatti et al. (2006), 41. Zinnecker et al. (1998), 42. Codella et al. (2007), 43. Smith et al. (2007), 44. Davis et al. (2008), 45. Stapelefeldt et al. (1991), 46. Carr (1993), 47. Hoddap & Ladd (1995), 48. Everett (1997, 49. Noriega-Crespo et al. (2002), 50. Khanzadyan et al. (2003), 51. Smith et al. (2003b), 52. Choi et al. (2006), 53. Aspin et al. (1994), 54. Hodapp et al. (2005), 55. Bally et al. (1993b), 56. Davis et al. (1994a), 57. Davis & Smith (1995), 58. Walawender et al. (2005), 59. Walawender et al. (2009), 60. Bally et al. (1993a), 61. Bachiller et al. (1994), 62. McCaughrean et al. (1994), 63. Eisloffel et al. (2003), 64. Salas et al. (2003), 65. O'Connell et al. (2005), 66. Walawender et al. (2006), 67. Yu et al. (1999), 68. Yamashita & Tamura (1992), 69. Davis et al. (1995), 70. Hayashi & Pyo (2009), 71. Varricatt et al. (2010), 72. van Langevelde et al. (1994), 73. Herbst et al. (2007), 74. Beck et al. (2008), 75. Moreira & Yun (1995), 76. Gómez et al. (1997), 77. Khanzadyan et al. - in prep., 78. Lucas et al. (2000), 79. Davis et al. (2007), 80. Davis et al. (1998), 81. Shepherd et al. (2003), 82. Shepherd et al. (2000), 83. Cesaroni et al. (2005), 84. Caratti o Garatti et al. (2008), 85. Kumar et al. (2002), 86. Jiang et al. (2004), 87. Davis & Smith (1996), 88. Cruz-González et al. (2007), 89. Khanzadyan et al. - in prep., 90. Movsessian et al. (2003), 91. Smith & Fischer (1992), 92. Tamura & Yamashita (1992), 93. Chen et al. (1999), 94. Chen et al. (2003), 95. Varricatt et al. (2005), 96. Porras et al. (2000), 97. Khanzdyan et al. (2004b), 98. Chakraborty et al. (2000), 99. Indebetouw et al. (2003), 100. Anandarao et al. (2004), 101. Miralles et al. (1997), 102. Hodapp (2007), 103. Fang & Yao (2004), 104. Reipurth et al. (2004), 105. Piché et al. (1995), 106. Yun et al. (2001), 107. Jiang et al. (2003), 108. Aspin (1998), 109. Li et al. (2008), 110. Wang et al. (2002), 111. Tokunaga (2004), 112. Wang et al. (2002), 113. Phelps & Ybarra (2005), 114. Eislöffel et al. (1994), 115. Micono et al. (1998), 116. Lorenzetti et al. (2002), 117. Caratti o Garatti et al. (2004), 118. De Luca et al. (2007), 119. Giannini et al.(2007), 120. Giannini et al. (2005), 121. Gredel (2006), 122. Yun et al. (1997), 123. Bourke (2001, 124. Brooks et al. (2003), 125. Persi et al. (2009), 126. Megeath & Tieftrunk (1999), 127. Persi et al. (1996), 128. Tachihara et al. (2007), 129. Wilking et al. (1997), 130. Davis et al. (1999), 131. Giannini et al. (2008), 132. Khanzadyan et al. (2004a), 133. Gómez et al. (2003), 134. Dent et al. (1995), 135. Grosso et al.(2001), 136. Ybarra et al. (2006), 137. Fuller et al. (1995), 138. Davis et al. (2004), 139. Todd & Ramsay Howat (2006), 140. Hodapp K.W. - private communication, 141. Hodapp (1999), 142. Herbst et al. (1997), 143. Djupvik et al. (2006), 144. Nurnberger et al. (2007), 145. Persi et al. (2003), 146. Hodapp (1998), 147. Gålfalk & Olofsson (2007b), 148. Davis et al. (1995), 149. Hodapp & Davis (2002), 150. Beuther et al. (2003), 151. Palacios & Eiroa (1999), 152. Hartigan et al. (2000), 153. Hiriart et al. (2004), 154. Cunningham (2009), 155. Nadeau et al. (1994), 156. Hartigan et al. (1996), 157. Goetz et al. (1998), 158. Eislöffel et al. (1996), 159. Ladd & Hodapp (1997), 160. Ayala et al. (2000), 161. Smith et al. (2003a), 162. Chen & Yao (2004), 163. Schultz et al. (1995), 164. Massi (2004), 165. Yao et al. (2000), 166. Chen et al. (2009), 167. Nisini et al. (2001), 168. Beltran et al. (2009), 169. Reach et al. (2009), 170. Birkmann et al. (2007), 171. Bally et al. (1995), 172. Fontani et al. (2004), 173. Salas et al. (1998), 174. Giannini et al. (2006), 175. Giannini et al. (2009), 176. Gómez et al. (2004), 177. Caratti o Garatti et al. (2009), 178. This paper, 179. Froebrich & Scholz (2003), 180. Ybarra et al. - in prep., 181. Ginsburg et al. (2009), 182. Davis et al. (2010).


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