Table 3
WSRT H i properties.
HVC name | AGC | RA+Dec | cz | W50 | θhf | SHI | NHI,peak | ||||
210′′ | 210′′ | 105′′ | 60′′ | 210′′ | 105′′ | 60′′ | |||||
J2000 | km s-1 | km s-1 | ′ | Jy km s-1 | 1019 atoms cm-2 | ||||||
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | ||||
|
|||||||||||
HVC214.78+42.45+47 | 198606 | 093002.8+163813 | 51 | 24 | 11.4 | 15.3 | 14.0 | 11.8 | 4.2 | 4.9 | 6.1 |
HVC204.88+44.86+147 | 198511 | 093017.2+241119 | 151 | 15 | 7.0 | 0.86 | 0.78 | ... | 0.59 | 0.98 | ... |
HVC205.83+45.14+173 | 198683 | 093212.8+233348 | 176 | 23 | 8.2 | 0.63 | 0.42 | ... | 0.46 | 1.2 | ... |
HVC217.77+58.67+96 | 208747 | 103710.0+203214 | 96 | 19 | 6.8 | 1.69 | 1.57 | ... | 1.1 | 1.6 | ... |
HVC212.68+62.39+64 | 208753 | 104931.8+235526 | 65 | 24 | 10.6 | 3.32 | 3.1 | ... | 0.93 | 1.4 | ... |
HVC230.27+71.10+76 | 219663 | 113422.1+201212 | 73 | 13 | 5.8 | 0.65 | 0.49 | ... | 0.68 | 1.1 | ... |
HVC235.38+74.79+195 | 219656 | 115123.7+203403 | 191 | 28 | 8.0 | 1.22 | 1.09 | ... | 0.67 | 1.2 | ... |
HVC271.57+79.03+248 | 229326 | 122735.5+173852 | 239 | 22 | 5.5 | 0.63 | 0.58 | ... | 0.63 | 1.0 | ... |
HVC276.53+79.84+255 | 229327 | 123223.6+175522 | 253 | 17 | 8.8 | 0.62 | 0.62 | ... | 0.38 | 0.88 | ... |
HVC028.09+71.87-142 | 249393 | ... | ... | ... | ... | ... | ... | ... | 0.34a | ... | ... |
HVC011.76+67.89+60 | 249525 | 141752.7+173240 | 47 | 18 | 6.8 | 5.12 | 4.85 | 4.64 | 3.6 | 4.8 | 5.4 |
HVC015.96+63.90+44 | 249565 | 143556.3+170847 | 29 | 18 | 5.4 | 1.69 | 1.74 | 1.6 | 1.8 | 2.9 | 4.0 |
Notes. Table columns are as follows: Col. 1: the HVC name of the source as for Table 1; Col. 2: AGC number as in Table 1; Col. 3: equatorial coordinates of the H i centroid (epoch J2000) for the 210′′ WSRT data, derived using the task maxfit in Miriad; Col. 4: heliocentric recessional velocity, derived from Gaussian fitting to the WSRT 210′′ spectrum; Col. 5: full width at half maximum of the WSRT 210′′ spectrum, derived from Gaussian fitting; Col. 6: effective half-flux radius in arcminutes, derived as discussed in Sect. 2.2; Col. 7: integrated flux density for each angular resolution, calculated as discussed in Sect. 2.2. The uncertainty is taken to be 10%; Col. 8: peak NHI for each angular resolution in units of 1019 atoms cm-2.
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