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Table 1.

LOFAR sample of ram-pressure-stripped galaxies in the Virgo cluster.

VCC NGC IC Morphology log M H I-def. Δvrad, M 87 Literature Comment
[log M] [km s−1]
(1) (2) (3) (4) (5) (6) (7) (8) (9)
241 3105 SW tail 7.89 0.41 −1439 B22 New radio tail, Hα tail
307 4254 N tail 10.39 0.06 1124 V05, H07, V12b, B18a, M09 RPS + tidal interaction
497 4302 Light N tail 10.44 0.50 −153 C07, V13, W12 New radio tail, H I tail
630 4330 S tail 9.52 0.92 321 C07, M09, V12a, V12b, V13, F18 H I tail, Hα tail
664 3258 W tail 8.20 0.57 −1713 New candidate
865 4396 NW tail 9.25 0.20 −1398 C07, V07, V10, M09 H I tail
873 4402 NW tail 10.04 0.83 −1049 CR05, V07, M09, V10, V12b H I tail, stripped dust
979 4424 Small S tail 10.17 0.98 −842 C07, V13, B18b H I tail, Hα tail/outflow,
radio deficient
1401 4501 NE tail 10.98 0.58 999 W07, V07, V10, V12b
1450 3476 Long W tail 9.02 0.66 −1112 B21 New radio tail, Hα tail
M87 side-lobes
1516 4522 Long NW tail 9.38 0.68 1037 V04, M09, V12b
1532 800 NE tail 9.07 1.00 1051 New candidate
1615 4548 N-S asymmetry 10.74 0.94 −802 V99, W07 Old stripping event
1690 4569 SW tail, outflows 10.66 1.05 −1503 M09, V12b, B16 Hα tail
1868 4607 Asymmetry 9.6 0 1.20 973 New candidate
1932 4634 SW tail 9.57 0.45 −1163 S18 New candidate, star-forming
object in the tail (S18)
1987 4654 Asymmetry 10.14 −0.05 −240 V03, V07, C07, W07, V10 H I tail, RPS and
tidal interaction

Notes. Columns 1–3 list the identifiers of the galaxies in the VCC, NGC and IC. Column 4 comments on the LOFAR morphology of the sources and Cols. 5–7 show the stellar mass (from Boselli et al. 2015), H I deficiency and the radial velocity relative to M 87 (taken from HyperLeda https://leda.univ-lyon1.fr/). In Cols. 8 and 9, we list the relevant literature and additional comments.

References. V99 – Vollmer et al. (1999); V03 – Vollmer (2003); V04 – Vollmer et al. (2004) CR05 – Crowl et al. (2005); V05 – Vollmer et al. (2005a); C07 – Chung et al. (2007); H07 – Haynes et al. (2007); W07 – Weżgowiec et al. (2007); V07 – Vollmer et al. (2007); M09 – Murphy et al. (2009); V10 – Vollmer et al. (2010), V12a – Vollmer et al. (2012a); V12b – Vollmer et al. (2012b), W12 – Weżgowiec et al. (2012); V13 – Vollmer et al. (2013); B16 – Boselli et al. (2016b); B18a – Boselli et al. (2018b); B18b – Boselli et al. (2018c); S18 – Stein et al. (2018); B21 – Boselli et al. (2021); B22 – Boselli et al. (2022).

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