2020AJ....159...37K


Query : 2020AJ....159...37K

2020AJ....159...37K - Astron. J., 159, 37-37 (2020/February-0)

Neutral hydrogen observations of low surface brightness galaxies around M101 and NGC 5485.

KARUNAKARAN A., SPEKKENS K., BENNET P., SAND D.J., CRNOJEVIC D. and ZARITSKY D.

Abstract (from CDS):

We present atomic hydrogen (H I) observations using the Robert C. Byrd Green Bank Telescope along the lines of sight to 27 low surface brightness (LSB) dwarf galaxy candidates discovered in optical searches around M101. We detect H I reservoirs in five targets and place stringent upper limits on the remaining 22, implying that they are gas-poor. The distances to our H I detections range from 7 to 150 Mpc, demonstrating the utility of wide-bandpass H I observations as a follow-up tool. The systemic velocities of three detections are consistent with that of the NGC 5485 group behind M101, and we suggest that our 15 nondetections with lower distance limits from the optical are associated with and have been stripped by that group. We find that the gas richness of confirmed M101 satellites are broadly consistent with those of the Milky Way satellites, as well as with those of satellites around other hosts of comparable mass, when survey completeness is taken into account. This suggests that satellite quenching and gas stripping proceed similarly around halos of similar mass, in line with theoretical expectations.

Abstract Copyright: © 2020. The American Astronomical Society. All rights reserved.

Journal keyword(s): Dwarf galaxies - Low surface brightness galaxies - H I line emission - Galaxy evolution

Simbad objects: 36

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Number of rows : 36
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 LEDA 2576103 G 13 43 07.27944 +58 13 39.9504           ~ 11 0
2 Z 272-13 AG? 13 54 45.602 +53 54 20.06   14.2       ~ 219 0
3 [MSB2017] dw1355+51 G? 13 55 11.0 +51 54 29           ~ 5 0
4 [BSC2017] Dw 9 LSB 13 55 44.6 +55 08 45           ~ 11 0
5 [BSC2017] Dw 38 LSB 14 01 17.6 +54 21 14           ~ 2 0
6 MATLAS-1692 LSB 14 02 20.0 +55 39 19           ~ 6 0
7 NAME M101 Group GrG 14 03 +54.3           ~ 112 1
8 [MVA2014] DF 3 LSB 14 03 05.7 +53 36 56   17.9       ~ 21 0
9 M 101 GiP 14 03 12.583 +54 20 55.50   8.46 7.86 7.76   ~ 3138 2
10 SMDG J1403450+535638 LSB 14 03 45.0 +53 56 40   18.9       ~ 21 0
11 MATLAS-1703 LSB 14 04 13.0 +55 43 35           ~ 4 0
12 [KRZ2015] M 101 dwD LSB 14 04 24.6 +53 16 19   19.2       ~ 7 0
13 MATLAS-1704 LSB 14 04 24.8 +55 06 14           ~ 6 0
14 [MVA2014] DF 5 LSB 14 04 28.1 +55 37 00           ~ 9 0
15 NGC 5473 GiG 14 04 43.2276404712 +54 53 33.499699368   12.5       ~ 156 0
16 NGC 5474 GiP 14 05 01.608 +53 39 43.95   11.28 10.79     ~ 475 1
17 MATLAS-1708 LSB 14 05 18.1 +54 53 52   20.2       ~ 9 0
18 NGC 5477 AG? 14 05 33.318 +54 27 37.85 13.94 14.36 14.01     ~ 224 1
19 SMDG J1406499+534430 LSB 14 06 49.9 +53 44 30   19.2       ~ 17 0
20 NGC 5485 LIN 14 07 11.3594809920 +55 00 06.084219996 14.34 13.82 12.22     ~ 267 0
21 MATLAS-1730 LSB 14 07 21.0 +55 03 51           ~ 7 0
22 MATLAS-1741 LSB 14 07 41.7 +54 35 19           ~ 6 0
23 SMDG J1407464+541525 LSB 14 07 46.4 +54 15 26           ~ 4 0
24 [BSC2017] Dw 13 LSB 14 08 01.2 +54 22 30           ~ 3 0
25 MATLAS-1752 LSB 14 08 33.7 +55 26 50           ~ 4 0
26 SMDG J1408374+541932 LSB 14 08 37.5 +54 19 31   19.8       ~ 20 0
27 SMDG J1408411+565536 LSB 14 08 41.0 +56 55 38           ~ 6 0
28 MATLAS-1754 LSB 14 08 43.7 +55 10 02   20.1       ~ 9 0
29 MATLAS-1755 LSB 14 08 45.8 +55 17 13           ~ 6 0
30 [BSC2017] Dw 26 LSB 14 08 50.4 +53 27 24           ~ 3 0
31 MATLAS-1774 LSB 14 10 20.0 +54 45 50           ~ 3 0
32 [MSB2017] dw1412+56 G? 14 12 11.0 +56 08 31           ~ 5 0
33 SMDG J1413016+551117 LSB 14 13 01.7 +55 11 16           ~ 5 0
34 SMDG J1416592+575441 LSB 14 16 59.0 +57 54 39           ~ 7 0
35 MCG+10-21-013 AG? 14 35 24.077 +57 15 21.24   17       ~ 91 0
36 [MSB2017] dw1446+58 G? 14 47 00.0 +58 34 04           ~ 5 0

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