Table B.1
PN-like objects with RP < −0.4 found in Gaia DR3.
| Name | Radius [″] | Density [arcmin−2] | Type | Reference for radius estimate |
|---|---|---|---|---|
| LMC-SMP-81 | 0.15 | 4.8 | PN | Stanghellini et al. (2003) |
| LMC-SMP-79 | 0.22 | 6.7 | PN | Stanghellini et al. (2003) |
| SMC-SMP-27 | 0.23 | 8.3 | PN | Stanghellini et al. (2003) |
| SMC-SMP-15 | 0.17 | 14.6 | PN | Stanghellini et al. (2003) |
| SMC-SMP-5 | 0.31 | 15.9 | PN | Stanghellini et al. (2003) |
| SMC-SMP-16 | 0.18 | 32.1 | PN | Stanghellini et al. (2003) |
| LMC-SMP-71 | 0.31 | 47.4 | PN? | Stanghellini et al. (2003) |
| LMC-SMP-34 | 0.32 | 68.1 | PN | Stanghellini et al. (2003) |
| LMC-SMP-80 | 0.21 | 71.3 | PN | Stanghellini et al. (2003) |
| LMC-SMP-48 | 0.2 | 74.5 | PN | Stanghellini et al. (2003) |
| PN G315.4+09.4 | 2.5 | 11.5 | PN | Stanghellini & Haywood (2010) |
| LMC-SMP-67 | 5.4 | 17.5 | PN | Reid & Parker (2006) |
| LMC-SMP-76 | 4.7 | 18.1 | PN | Reid & Parker (2006) |
| LMC-SMP-37 | 4.9 | 20.0 | PN | Reid & Parker (2006) |
| LMC-SMP-55 | 5.7 | 20.0 | PN | Reid & Parker (2006) |
| He 2–25 | 2.2 | 23.2 | PN | Stanghellini & Haywood (2010) |
| PN G319.0−04.1 | 6.0 | 23.3 | PN | Le Dû et al. (2022) |
| LMC-SMP-23 | 5.7 | 26.7 | PN | Reid & Parker (2006) |
| LMC-SMP-75 | 5.0 | 29.3 | PN | Reid & Parker (2006) |
| LMC-SMP-78 | 5.7 | 36.9 | PN | Reid & Parker (2006) |
| LMC-SMP-36 | 3.8 | 39.1 | PN | Reid & Parker (2006) |
| LMC-SMP-56 | 5.0 | 42.7 | PN | Reid & Parker (2006) |
| LMC-SMP-63 | 5.0 | 46.5 | PN | Reid & Parker (2006) |
| LMC-SMP-38 | 6.6 | 46.8 | PN | Reid & Parker (2006) |
| LMC-SMP-77 | 6.0 | 47.1 | PN | Reid & Parker (2006) |
| LMC-SMP-73 | 5.8 | 52.5 | PN? | Reid & Parker (2006) |
| LMC-SMP-26 | 5.7 | 71.0 | PN | Reid & Parker (2006) |
| LMC-SMP-29 | 6.0 | 76.1 | PN | Reid & Parker (2006) |
| PN G356.9−05.8 | 3.4 | 87.2 | PN | Stanghellini & Haywood (2010) |
| LMC-SMP-64 | 6.0 | 94.2 | PN | Reid & Parker (2006) |
| MGPN LMC 39 | 4.4 | 122.5 | PN | Reid & Parker (2006) |
| LMC-SMP-47 | 5.0 | 149.9 | PN | Reid & Parker (2006) |
| EC 05147–5727 | – | 0.6 | Cataclysmic variable | |
| J132856.71+310846.0 | – | 0.6 | Cataclysmic variable | |
| [M94b] 48 | – | 1.6 | PN candidate | |
| [M94b] 54 | – | 1.6 | PN candidate | |
| LMC-SMP-3 | – | 1.9 | PN | |
| SMC-SMP-4 | – | 2.5 | PN | |
| SMC-SMP-28 | – | 2.5 | PN | |
| WDJ214206.81+030322.26 | – | 2.5 | WD | |
| LMC-SMP-61 | – | 3.8 | PN | |
| [M94b] 49 | – | 3.8 | PN | |
| J174506.57–020844.1 | – | 4.5 | QSO | |
| He 2-375 | – | 4.5 | PN | |
| SMC-SMP-17 | – | 4.5 | PN | |
| LMC-SMP-94 | – | 4.8 | PN | |
| MGPN LMC 45 | – | 4.8 | PN | |
| LMC-SMP-2 | – | 5.7 | PN | |
| LM 1-60 | – | 6.0 | PN candidate | |
| PN G053.6−12.3 | – | 6.4 | PN candidate | |
| 2MASS 382453513 | – | 6.7 | AGN candidate | |
| Gaia DR3 #6128295187479810560 | – | 7.0 | stellar | Previously unknown PN? |
| LMC-SMP-85 | – | 7.6 | PN | |
| LMC-SMP-1 | – | 8.3 | PN | |
| LMC-SMP-5 | – | 8.3 | PN | |
| LMC-SMP-84 | – | 14.3 | PN | |
| V* V339 Del | – | 14.3 | Classical Nova | |
| He 2–90 | – | 15.0 | PN | |
| [MA93] 1721 | – | 15.6 | Em* | |
| V* V2659 Cyg | – | 16.2 | Classical Nova | |
| SMC-SMP-6 | – | 16.9 | PN | |
| Gaia DR3 #4663598364758836992 | – | 16.9 | stellar | Previously unknown PN? |
| WDJ172916.00–525338.87 | – | 17.8 | WD | |
| J052744.6–665300 | – | 19.7 | stellar | |
| Gaia DR3 #4660554298082054400 | – | 20.0 | stellar | Previously unknown PN? |
| LMC-SM-62 | – | 20.0 | PN | |
| V* V1016 Cyg | – | 20.4 | PN?/symbiotic | |
| He 2-437 | – | 20.7 | PN | |
| LMC-SMP-8 | – | 21.3 | PN | |
| V* V2944 Oph | – | 21.3 | Classical nova | |
| Gaia DR3 #4660478947196927232 | – | 22.0 | stellar | Previously unknown PN? |
| Lin 49 | – | 25.1 | PN | |
| PN MaC 1–15 | – | 26.1 | PN candidate | |
| J054519−711603 | – | 26.7 | PN | |
| LMC-SMP-74 | – | 28.0 | PN | |
| PN G342.8+04.1 | – | 29.6 | PN | |
| J053048.9−671010 | – | 31.5 | stellar | |
| J185938.6−091102 | – | 32.8 | stellar | |
| LMC-SMP-89 | – | 37.2 | PN | |
| LM 1–14 | – | 39.8 | PN candidate | |
| PN G007.5+04.3 | – | 43.6 | PN | |
| LMC-SMP-51 | – | 50.0 | PN | |
| Gaia DR3 #5836588052566682880 | – | 51.9 | stellar | Previously unknown PN? |
| SMC-SMP-21 | – | 73.5 | PN | |
| G354.98−02.87 | – | 85.6 | Symbiotic | |
| V* V5667 Sgra | – | 117.5 | Dwarf nova | |
Notes. aPN-like objects found using our search for compact, zero-redshifted emission-line sources (orange lines in the bottom panels of Fig. 4). The first section of this table shows objects with radii ≤ 0.″5, sorted by stellar field density (local number density of Gaia sources with Gmag<19mag). The second section shows objects with radii > 0.″5. The third section shows objects without size estimate in HASH.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.