Forums

List of all stars, brown dwarves and planets within 10 parsecs

Sort:
Yigor

I use SIMBAD database. openings There are 533 astronomical objects within 10 parsecs. peshka

N°  |   Name                                                     | Parallax | Visual magnitude | Spectral type

1b NAME Proxima Centauri b 768.5004   planet
1c NAME Proxima Centauri c 768.5004   planet
1d NAME Proxima d 768.5004   planet
1 NAME Proxima Centauri 768.0665 11.13 M5.5Ve
2A * alf Cen A 743 0.01 G2V
2B * alf Cen B 743 1.33 K1V
2 * alf Cen 742 -0.1 G2V+K1V
3 Gaia DR2 1824801659879180544 739.2807   ~
4b GJ 699 b 547.4506   ~
4 NAME Barnard's star 546.9759 9.511 M4V
5 NAME Luhman 16 496 16.20 L7.5+T0.5
523 WISEA J085510.74-071442.5 448   Y2
158 Wolf 359 415.1794 13.507 dM6
119 Wolf 359b 415.1794   ~
490 Wolf 359c 415.1794   ~
401 GJ 411 c 392.7529   ~
214 HD 95735 392.7529 7.520 M2+V
132 HD 95735b 392.7529   ~
461 * alf CMa 379.21 -1.46 A0mA1Va
354 G 272-61 375 12.08 M5.5V+M6V
375 * alf CMa B 374.4896 8.44 DA1.9
395 G 272-61B 373.8443   M6V
446 G 272-61A 367.7119   M5.5V
508 WISE J154151.65-225024.9 351   Y0
453 Ross 154 336.0266 10.43 M3.5Ve
506 Ross 248 316.4812   M5.0V
258 * eps Eri b 310.94   ~
527 * eps Eri c 310.94   ~
174 * eps Eri 310.5773 3.73 K2V
178 HD 217987b 304.2190   ~
194 HD 217987c 304.2190   ~
456 HD 217987d 304.2190   ~
340 HD 217987 304.1354 7.39 M2V
254 Ross 128b 296.3073   ~
147 Ross 128 296.3053 11.153 dM4
21 V* EZ Aqr 293.600 12.38 M5V
413 WISE J035000.32-565830.2 291   Y1
99 * 61 Cyg B 286.0054 6.03 K7V
360 * 61 Cyg A 285.9949 5.21 K5V
247 * alf CMi 284.56 0.37 F5IV-V+DQZ
268 HD 173739 283.8401   M3V
399 HD 173740 283.8378   M3.5V
138 V* GX And 280.7068   M2V
203 V* GQ And 280.6947 11.04 M3.5V
87 GJ 15 Ab 280.6902   ~
428 GJ 15 Ac 280.6902   ~
196 G 51-15 279.2496   M6.5Ve
219 * eps Ind 274.8431 4.69 K5V
349 * eps Ind b 274.8048   ~
310 * tau Cet b 273.96   ~
384 * tau Cet c 273.96   ~
297 * tau Cet d 273.96   ~
6 * tau Cet e 273.96   ~
133 * tau Cet f 273.96   ~
493 * tau Cet g 273.96   ~
17 * tau Cet h 273.96   ~
80 * tau Cet 273.8097 3.50 G8V
25 NAME L 372-58b 272.2446   ~
355 NAME L 372-58c 272.2446   ~
30 NAME L 372-58d 272.2446   ~
476 L 372-58 272.1615 13.07 M5.5V
465 * eps Ind B 270.6580 24.12 T1V+T6V
151 NAME YZ Cet b 269.3628   ~
488 NAME YZ Cet c 269.3628   ~
426 NAME YZ Cet d 269.3628   ~
470 V* YZ Cet 269.0573 12.074 M4.0Ve
342 BD+05 1668 264.1269 9.872 M3.5V
411 BD+05 1668b 264.1269   ~
186 BD+05 1668c 264.1269   ~
377 GJ 273 d 264.1269   ~
319 GJ 273 e 264.1269   ~
172 NAME Teegarden's Star b 261.0147   ~
492 NAME Teegarden's Star c 261.0147   ~
505 NAME Teegarden's Star 260.9884   dM6
293 SCR J1845-6357B 259.45   ~
86 HD 33793b 254.2263   ~
321 HD 33793c 254.2263   ~
372 HD 33793 254.1986 8.853 M1VIp
273 V* AX Mic 251.9124 6.68 M1V
324 WISE J053516.80-750024.9 250   Y1:+
8 HD 239960B 249.9668   M4V
52 HD 239960 249.94   M3
162 SCR J1845-6357 249.6651 17.40 M8.5V
392 HD 239960A 249.3926 11.41 M3V
187 DENIS J104814.6-395606 247.2156 17.532 M8.5Ve:
61 WISE J072227.27-054029.9 246.00   T9
415 Gaia DR2 4129144660321847040 243.6718   ~
185 Ross 614 242.9659 11.071 M4.5V
223 WISE J041022.71+150248.4 233   Y0
28 BD-12 4523b 232.2095   ~
429 BD-12 4523c 232.2095   ~
433 BD-12 4523d 232.2095   ~
517 BD-12 4523 232.1390 10.072 M3V
454 Wolf 28 231.7800 12.374 DZ7.5
7 Wolf 424 A 231.1185   ~
200 HD 225213 230.0970 8.562 M2V
386 Wolf 424 227.9 12.467 M5.5V
169 V* TZ Ari 223.7321 12.298 M4.5V
106 GJ 9066 b 223.6349   ~
473 GJ 9066 c 223.6349   ~
430 Wolf 424 B 223.4775   ~
1 CD-46 11540b 219.8012   ~
412 BD+68 946 219.7898   M3.0V
160 BD+68 946b 219.7807   ~
221 GJ 687 c 219.7807   ~
231 CD-46 11540 219.6463 9.407 M3V
170 LP 731-58 219.3302 15.784 M6.5V
380 LAWD 37 215.6753 11.513 DQ
507 G 208-45 214.5745 13.99 M6V
301 BD-15 6290 214.0380 10.192 M3.5V
397 BD-15 6290b 213.8669   ~
409 BD-15 6290c 213.8669   ~
322 BD-15 6290d 213.8669   ~
307 BD-15 6290e 213.8669   ~
282 G 208-44 213.1329 13.126 M5.5Ve
77 L 143-23 206.9698 13.920 M5.5V
29 G 158-27 206.3500 13.837 M5.5V
267 DENIS J025503.3-470049 205.4251 22.921 L9
246 HD 88230 205.3148 6.61 K6VeFe-1
524 BD+44 2051 203.8876   M1.0V
110 BD+44 2051B 203.8323 14.45 M6.0V
107 WISE J163940.83-684738.6 202.3   Y0pec
532 HD 204961b 201.4073   ~
266 HD 204961c 201.4073   ~
253 BD+20 2465 201.4064 9.52 dM3
435 HD 204961 201.3252 8.672 M2/3V
513 * omi02 Eri b 200.62   ~
248 G 158-50 200.53 11.483 M4V
98 CD-44 11909b 199.7031   ~
120 CD-44 11909c 199.7031   ~
240 CD-44 11909 199.6944 10.946 M3.5
407 * omi02 Eri B 199.6911 9.53 DA2.9
208 * omi02 Eri 199.6080 4.43 K0V
67 * omi02 Eri C 199.4516 11.17 M4.5V
388 V* EV Lac 197.9573 10.26 M4.0Ve
359 * 70 Oph 196.72 4.03 K0-V
239 G 9-38B 196.2619 13.75 M7V
236 2MASS J09393548-2448279 196.0   T8
92 * 70 Oph B 195.8563 6.07 K4V
475 * 70 Oph A 195.5674   K0V
165 * alf Aql 194.95 0.76 A7Vn
485 G 9-38A 194.1443 13.93 M8Ve
264 2MASS J15065257+7027247 193.9412   T6
393 G 99-49 192.0135 11.31 M3.5Ve
271 2MASS J08173001-6155158 191.8362   T6
347 G 254-29 190.3251   M4.0V
466 G 9-38 190   M7V+M7V
184 UCAC4 195-119117 187.7290   M6.5
389 NAME HD 101847BC 187.20   ~
149 LP 656-38 186.0466 12.196 M4.0Ve
521 NAME LP 656-38b 186.0231   ~
139 NAME LP 656-38c 186.0231   ~
530 2MASS J02540788+0223563 185   T8.0
431 HD 119850 183.9962 8.50 M2V
23 EGGR 180 181.2730   DC5
335 G 175-34 181.2438 10.98 M4.0V
451 GJ 251 b 179.1642   ~
227 HD 265866 179.0629   M3V
37 LP 816-60 177.9312 11.458 M4V
11 2MASS J11145133-2618235 176.8   T7.5
20 WISEP J174124.25+255319.5 176   T9
249 LSR J1835+3259 175.7930   M8.5V
233 HD 36395 175.3131 7.968 M1.5Ve
47 2MASSI J0415195-093506 174.34   T8.0
74 HD 42581b 173.6955   ~
71 HD 42581c 173.6955   ~
320 HD 42581 173.5740 8.125 M1V
292 * sig Dra 173.4939 4.680 K0V
326 HD 42581B 173.19   T6.5
312 Ross 47 172.6762 11.509 M4V
468 HD 131977b 170.0112   ~
91 HD 131977 169.8843 5.72 K4V
210 L 205-128 169.8042 10.783 M3.5V
13 GJ 570 D 169.30   T8
84 L 347-14 169.2351 12.23 M4.5
497 V* BR Psc 169.2163 8.993 dM1
294 HD 180617b 169.1590   ~
325 HD 180617 169.0615 9.115 M3-V
414 CD-40 9712 168.9965 9.311 M2.5V
105 VB 10 168.9537 17.30 M8V
385 * eta Cas 168.8322 3.44 F9V
477 HD 131976 168.77 8.065 M1.5V
270 * eta Cas B 168.7186 7.51 K7Ve
362 * 36 Oph 168.54   K2V+K1V
22 * 36 Oph B 168.1303 5.03 K1V
285 * 36 Oph A 168.0031 5.08 K2V
135 V* V2215 Oph 167.9617 6.34 K5V
421 HD 155876 167.29 9.523 M3V
250 V* YZ CMi 166.9769 11.225 M4.0Ve
64 HD 191408 166.3272 5.32 K2.5V
103 * e Eri 165.5242 4.27 G6V
503 * e Eri b 165.47   ~
410 * e Eri c 165.47   ~
274 * e Eri d 165.47   ~
478 * e Eri e 165.47   ~
331 * e Eri f 165.47   ~
318 * e Eri g 165.47   ~
339 V* QY Aur 165.2147 11.52 M4.5Ve
226 * del Pav 163.9544 3.56 G8IV
364 SIMP J013656.5+093347.3 163.4478   T2.0
256 2MASSI J0937347+293142 163.39   T6
467 HD 191849 162.2171 7.966 M0V
332 BD+19 5116 161.76 10.165 M4+M5
522 HD 152751 161.41 9.023 M3.5Ve
10 EGGR 372 160.9952   DQ9P
514 BD-11 3759 159.9225 11.317 M3.5V
338 BD+19 5116B 159.9085   M4.0Ve
112 BD+19 5116A 159.6634 10.173 M3.5Ve
458 BD-07 4003b 158.7492   ~
81 BD-07 4003c 158.7492   ~
512 BD-07 4003d 158.7492   ~
436 BD-07 4003e 158.7492   ~
416 BD-07 4003f 158.7492   ~
348 BD-07 4003g 158.7492   ~
483 BD-07 4003 158.7183 10.560 M3V
245 HD 79210 157.8879   K7V
499 HD 79211 157.8825   M0V
434 LP 368-128 157.2686 16.100 M6.5Ve
97 2MASS J15031961+2525196 155.7758   T5.5
427 LP 944-20 155.5982 18.69 M9.5Ve
140 EGGR 45 155.2373 14.45 DZ11
422 V* GL Vir 154.6999 13.90 M4.5Ve
122 NAME G 202-48b 154.4710   ~
343 WISE J220905.73+271143.9 154.410   Y0:
370 G 202-48 154.3503 10.07 M1.5V
391 VB 8 153.9659 16.916 M7Ve
291 Wolf 629 153.8754 11.759 M3.5V
19 L 100-115 153.7593 12.78 M4.0V
153 HD 219134b 153.0808   ~
16 HD 219134c 153.0808   ~
302 HD 219134d 153.0808   ~
57 HD 219134e 153.0808   ~
4 HD 219134f 153.0808   ~
141 HD 219134g 153.0808   ~
212 HD 219134h 153.0808   ~
533 WISEP J031325.96+780744.2 153   T8.5
83 HD 219134 152.8640 5.570 K3V
32 L 471-42 150.0781 12.74 M4.0V
379 * ksi Boo 148.98 4.593 G7Ve+K5Ve
183 Ross 104 148.1986 10.020 M4V
471 * ksi Boo B 148.1793 6.816 K5Ve
115 * ksi Boo A 148.0695 4.675 G7Ve
102 Ross 619 147.7218 12.834 M4.5V
117 G 41-14 147.66 10.98 M3.5V
66 Ross 775 147.4958 10.303 M3.0V
367 NAME Scholz's star 147   M9.5+T5
515 2MASS J19284155+2356016 146.4067   T6
480 HD 156384 146.29 5.89 K3V+K5V
281 BD-17 588A 145.6922 10.529 M3.0
104 HD 216899 145.6234 8.638 M1.5V
487 NAME BD-17 588Ab 145.5466   ~
76 NAME BD-17 588Ac 145.5466   ~
95 WISE J035934.06-540154.6 145   Y0
205 WISE J205628.91+145953.2 144   Y0
259 Wolf 358 143.5391 11.675 M4V
366 NAME GJ 393 b 142.1885   ~
314 BD+01 2447 142.0951 9.650 dM2
438 HD 199305 142.0543   M1.0V
262 LSPM J2146+3813 141.8946   M5V
176 LP 914-54 141.7891 17.141 M7.0Ve
374 2MASS J05212615+1025328 141.2   T7.5
275 L 230-188 140.6961 13.58 M3.5
204 NAME BD-17 588BC 139.70 10.59 M2.5V
124 G 157-77 139.3389 14.69 M5.0Ve
376 WISEA J082507.37+280548.2 139.020   Y0.5
455 V* BX Cet 138.4371   M3.5V
276 HD 16160 138.3400   K3V
383 2MASS J08354256-0819237 138.3147   L6.5
65 L 788-34 138.2280 13.30 M4.5Ve
525 HD 156384C 138.0663 10.22 M1.5V
202 2MASS J06073908+2429574 138.0616   L9
213 HD 156384Cb 138.0171   ~
171 HD 156384Cc 138.0171   ~
447 HD 156384Cd 138.0171   ~
40 HD 156384Ce 138.0171   ~
195 HD 156384Cf 138.0171   ~
350 HD 156384Cg 138.0171   ~
284 HD 156384Ch 138.0171   ~
199 2MASSW J1507476-162738 134.9474 22.136 L5V
58 G 161-7 134.9 13.804 M5.0V
189 HD 4628 134.4948 5.74 K2.5V
27 Wolf 922 134.0831 12.006 M4.5V
14 * bet Hyi 134.07 2.79 G0V
209 G 24-16 133.8113   M4.5V
373 WISE J140518.39+553421.3 133   Y0(pec?)
9 Gaia DR2 6702242043883732864 132.7692   ~
191 G 203-47 131.5996 13.671 M3.5V
75 V* TW PsA 131.5525 6.48 K4Ve
177 G 141-36 131.2790   M5.0V
462 2MASS J20005017+3629465 131.2   T8
498 BD+11 2576 131.1013 9.029 M1.0V
357 G 258-33 130.8531   M4.5Ve
242 * 107 Psc 130.8234 5.24 K1V
277 L 499-56 130.4186   M3.0V
12 * mu. Cas 130.2881 5.17 G5Vb
48 * alf PsA C 130.2707 12.624 M4.0Ve
443 * alf Lyr 130.23 0.03 A0Va
234 V* VX Ari 130.1956 10.563 dM3
313 * alf PsA 129.81 1.16 A4V
345 * alf PsA b 129.81   ~
341 V* AN Sex 129.7544 9.264 M2V
228 HD 157881 129.6459 7.56 K7V
449 SIPS J1259-4336 129.4288   M8:
481 LP 881-64 129.3167 15.338 M5.5/6Ve+M8.5Ve+M9/9.5V
516 G 192-13 129.3014   M4.0V
419 HD 165222 129.2184 9.360 M0V
295 G 109-35 128.9866   M5.0Ve
94 G 227-22 128.3057   M5.0V
529 WISEP J180026.60+013453.1 128.0546   L7.5
69 * p Eri 127.84   K2V+K2V
201 G 202-45 127.4785   M3.0V
51 2MASS J07290002-3954043 126.3   T8pec
62 G 154-44 125.4509 13.48 M4.0Ve
440 SCR J0740-4257 125.3028 13.835 M4.5
363 CD-44 3045 124.85 10.846 M3.5V
306 CD-44 3045A 124.5695 11.48 M3
142 CD-44 3045B 124.3569 11.29 M3
63 G 122-49 124.3378   M4.5V
387 L 399-68 124.1851 12.239 M3V
337 * chi Dra 124.11 3.580 F7V
378 * pi.03 Ori 123.94 3.190 F6V
88 TOI-1827.01 123.8215   ~
300 Wolf 437 123.7756 11.395 M3.5V
125 2MASSW J2148162+400359 123.6752   L7
252 G 262-15 123.6547   M3V
432 G 13-22 123.6430   M4.5Ve
287 L 674-15 123.2033 12.13 M3.5V
263 EGGR 290 123.1989 14.13 DA8P
371 IRAS 21500+5903 123.0568 10.64 M3.9
152 BD+18 3421b 122.5609   ~
358 BD+18 3421 122.5546 9.577 M1.5V
356 LAWD 26 122.4130 14.09 DA9.0
116 * p Eri A 122.1088 5.685 K2V
46 * p Eri B 122.0035 5.797 K2V
154 L 173-19 121.7084 12.90 ~
73 HD 217357 121.4724 7.869 K7+Vk
272 Ross 318 121.4598   M3.0V
261 CD-68 47 121.4487 9.824 M2.5V
510 * mu.02 Her B 120.3979   ~
305 G 207-16 120.200 11.26 M3V
469 LAWD 96 120.0143 13.05 DAP5.8
381 * mu.01 Her 119.9248 3.42 G5IV
299 * mu.02 Her A 119.8871   ~
161 * mu.02 Her 119.7908   M3.5V
472 Wolf 489 119.7566   DC9
93 G 227-29 119.7519   M4.0V
114 G 130-4 119.5794 12.67 M4.5Ve
251 HD 32450A 119.5737 8.66 K7
197 SCR J1138-7721 119.3419 14.780 M5.0V
137 HD 32450 119.3399 8.317 K7V
518 SCR J1546-5534 119.0962   M7.5
198 HD 32450B 118.8250 10.60 ~
484 UCAC4 747-070768 118.1551   DAH
280 * bet CVn 118.0266 4.25 G0V
39 Ross 64 117.7263   M4V
89 CD-37 10765B 117.6791   M5:
45 CD-37 10765 117.4716 10.586 M3V
437 CD-32 5613 117.3961 11.85 DA5.5
333 * 61 Vir 117.1726 4.740 G6.5V
220 EGGR 453 117.1388 15.66 DZ13
127 Wolf 461 117.0327   M4.5Ve
145 * 61 Vir b 116.89   ~
316 * 61 Vir c 116.89   ~
44 * 61 Vir d 116.89   ~
496 G 89-32 116.60 13.24 M4.5V
482 L 49-19 116.3134 10.377 M3V
394 V* CD Cet 116.2678 14.001 M4.5V
181 * zet Tuc 116.1826 4.23 F9.5V
118 NAME CD Cet b 116.1536   ~
150 LP 502-56 116.0425   M5.5V
164 LP 666-9 115.4876 18.959 M9Ve
217 * chi01 Ori 115.43 4.40 G0V
328 V* AP Col 115.3982 12.96 M5
398 SIPS J1141-3624 115.0835 13.105 M5
108 G 19-7 114.9158 12.25 dM4
41 LP 991-84 114.604 14.403 M4.5V
188 * ksi UMa B 114.4867 4.77 G2V
317 * ksi UMa Bb 114.4867   ~
224 LSPM J0036+1821 114.4735   L3.5
36 HD 50281 114.3547 6.57 K3.5V
448 HD 50281B 114.2911 10.05 M2.5V
502 SCR J0630-7643 114.16 14.82 M6Ve
18 MCC 135 114.0854 9.802 M1.5V
509 * 41 Ara 113.7513 5.48 G9V
156 HD 192310b 113.6481   ~
72 HD 192310c 113.6481   ~
53 BD-05 5715b 113.6000   ~
235 BD-05 5715c 113.6000   ~
38 HD 192310 113.4872 5.723 K2+V
121 BD-05 5715 113.4447 10.366 M3.5V
131 * 41 Ara B 113.2858 8.69 M0VpCa-3Cr-1
229 Ross 730 113.2521 10.774 M2.0V
445 HD 349726 113.2228 10.771 M2V
123 * ksi UMa 113.2 3.79 F8.5:V+G2V
144 WISE J111838.70+312537.9 113.2   T8.5
243 L 32-8 113.1318 11.419 M3V
406 L 32-9 113.1304 10.484 M2V
26 HD 32147 113.0715 6.21 K3+V
255 NAME WISEP J121756.91+162640.2b 113   ~
126 WISE J121756.90+162640.8 113   T9+Y0
452 G 111-47 112.9927 13.912 M3.5V
424 V* FL Aqr 112.9867 11.49 M3.5V
168 NAME HIP 60559 b 112.7372   ~
232 Ross 695 112.6740 11.272 dM2.0
130 SCR J0630-7643A 112.6584   ~
90 LEHPM 3396 112.6100   M9
78 SCR J0630-7643B 112.5988   ~
526 Gaia DR2 2090670890062670080 112.5653   ~
113 V* AK Lep 112.4661 6.15 K3
352 V* FK Aqr 112.3859 9.083 M0Vep
311 * gam Lep 112.2960 3.60 F6V
43 CD-48 12943 112.12   ~
315 G 113-20 111.8698 10.091 M2.0V
157 G 193-27 110.8263 13.29 M5.0V
330 CD-31 9113b 110.2908   ~
79 CD-31 9113c 110.2908   ~
511 CD-31 9113d 110.2908   ~
34 V* SZ UMa 110.2305   M2V
444 CD-31 9113 110.1711 9.813 M2V
425 2MASSI J0727182+171001 110.14   T7.0
450 * del Eri 110.0254 3.54 K0+IV
289 HD 115953 109.9837 8.54 M2V
31 LP 469-206 109.9500   M5.0Ve
206 EGGR 246 109.9276 14.60 DQ9
404 V* V374 Peg 109.8548   M3.5Ve
418 2MASS J06523073+4710348 109.7651   L3.5+L6.5
479 WT 460 109.7323   M5.5e
193 ULAS J141623.94+134836.3 109.70   T7.5p
382 * kap01 Cet 109.41 4.85 G5V
35 LAWD 25 109.3440 13.061 DZQA6
304 LP 783-2 109.2545 16.696 M6.5Ve
369 2MASS J03552337+1133437 109.1381   L5gamma
298 WISEP J213456.73-713743.6 109.1   T9pec
230 HD 103095 109.0296 6.45 K1V_Fe-1.5
279 Ross 1015 108.7903 13.896 M4V
244 * bet Com 108.7250 4.25 F9.5V
368 WISE J071322.55-291751.9 108.7   Y0
269 2MASS J17502484-0016151 108.5809   L5.5
155 L 737-9 108.3254 10.302 M3.5V
190 LP 776-46 108.2732 11.735 M3V
180 LP 469-67 108.2582   M5.5V
329 CFBDS J005910-011401 108.20   T9.0
439 * gam Pav 108.0102 4.22 F9VFe-1.4CH-0.7
423 G 112-50 107.8488 13.26 M4.5V
109 WISEP J232519.54-410534.9 107.8   T9pec
344 2MASS J14162408+1348263 107.7375   L5
400 HD 102365b 107.6210   ~
309 HD 102365B 107.4237 15.43 M4V
163 GAT 1367 107.3873 15.68 M6.0V
24 HD 102365 107.3024 4.88 G2V
173 BD-18 359 107.2972 10.189 M2.5
442 2MASS J18212815+1414010 107.0339   L5
59 2MASS J03400942-6724051 106.8602   L7::
323 Ross 837 106.8404   M3.5Ve
100 CD-30 731 106.6096 12.167 M2.5+V
257 EGGR 41 106.3390 14.10 DQ8
405 Wolf 1062 106.2794 11.143 M3.5V
215 TOI-731.01 106.2112   ~
464 CD-45 5378 106.1727 9.979 M1.0
182 BD-17 588 106.16   M3.5+M3.0
278 L 678-39 105.9789 10.906 M2.5V
70 GJ 357 e 105.8830   ~
50 NAME L 678-39b 105.8830   ~
474 NAME L 678-39c 105.8830   ~
408 NAME L 678-39d 105.8830   ~
457 1RXS J115928.5-524717 105.7052   M9Ve
390 G 222-11 105.6903   M2.5V
491 HD 285968b 105.5627   ~
56 PM J18057-1422 105.5229   M5.5V
403 WISE J114156.71-332635.8 105.5   Y0
463 HD 285968 105.4275 9.951 M2.5V
148 2MASS J00345157+0523050 105.4   T6.5
5 GJ 3512 b 105.3856   ~
520 GJ 3512 c 105.3856   ~
134 CD-51 6859 105.3467 10.663 M3V(e)
365 G 234-45 105.2935   dM5.5
290 BPS CS 22879-0089 105.1555 13.53 ~
128 L 35-12 105.0336 13.10 M4.5V
216 G 192-15 104.9590   M5.0V
336 G 144-25 104.9190 13.41 M4.5V
54 BD+43 2796 104.9147 10.49 M2V
175 G 42-24 104.7638   M4.0Ve
396 * 20 Crt B 104.6570 15 DC
286 * 20 Crt 104.6133 5.98 K0V
260 Wolf 1069 104.4415   dM5.0
55 * 61 UMa 104.4252 5.34 G8V
353 PM J20502-3424 104.1310 13.88 M5e
2 CD-40 5404 104.0957 10.694 M3V
500 Wolf 227 103.5008   M5V
42 2MASS J14053729+8350248 103.4474   L8
33 CD-48 11837 103.3081 10.127 M1.5V
494 CD-48 11837B 103.2027   M3V
308 L 768-119 103.1798 11.855 M3
111 V* AU Mic 102.9432 8.627 M1VeBa1
420 L 88-59 102.9078 13.90 DA8.1
207 NAME AU Mic b 102.8295   ~
296 NAME AU Mic c 102.8295   ~
528 2MASS J22361685+5105487 102.8   T5
15 2MASS J20304235+0749358 102.7966   T1.5
241 G 119-36 102.7521   M5V
459 2MASS J02572581-3105523 102.6993   L8.5
159 LP 655-48 102.5942 17.79 M7.5Ve
218 Ross 905b 102.5015   ~
495 Ross 905c 102.5015   ~
288 Ross 905d 102.5015   ~
334 Ross 905 102.3014 10.613 M3V
129 G 268-110 102.2827 14.47 dM5.0
501 V* AT Mic B 101.9724 11.34 M4.5Ve
166 2MASSW J1515008+484742 101.9645   L6.5
49 HD 151288 101.5615 8.11 K7.5Ve
101 CFBDS J213926+022023 101.5   L8.5+T3.5
441 BD+61 195b 101.4650   ~
85 BD+61 195 101.4238   M1.5V
531 Wolf 47 101.3724 13.21 M5V
3 BD+66 34A 101.0864 10.327 M2V
192 * 12 Oph 101.0719 5.77 K1V
68 UPM J0815-2344 101.0408 12.30 ~
82 G 203-42 100.9274   M5.0V
417 HD 232979 100.9161 8.648 M0.5V
460 G 48-20 100.9033 11.710 M3.5V
361 WISE J033605.05-014350.4 100.900   Y0
346 V* AT Mic A 100.7921 10.36 M4.5Ve
402 G 160-28 100.7299 12.843 M3V
327 G 184-19 100.6850   M4.5V
225 L 403-34 100.6025 13.003 M5e
265 Gaia DR3 478823780455331968 100.5826   ~
143 G 184-19B 100.5553 14.40 M4.5Ve
504 BD+16 2708 100.5243 10.150 M3V
211 BD+66 34B 100.3966 12.19 M3V
237 LP 98-79 100.3110 17.88 M6.5V
303 WISE J182831.08+265037.7 100.210   Y0
222 G 36-24 100.1465   M3.5Ve
351 HD 260655 100.0232 9.593 M0.0V
Yigor

Distance in parsecs is calculated as 1000/parallax.

Distance in light-years = 3.261563777 * distance in parsecs. settings

Rigelianoid

Nice work!

How did you do the spectral types?

Background is that I tried to brute-force-fit BmV and UmB to Planck curves to get a better fit for T_eff than by using Ballasteros et al. Was meant for a 3D-model of the Orion Arm I use for "navigation" in my science fiction saga.

(That is based on the second HIPPARCOS reduction parallaxes, not GAIA. Yet.)

Yigor
Rigelianoid wrote:

Nice work!

How did you do the spectral types?

Background is that I tried to brute-forse-fit BmV and UmB to Planck curves to get a better fit for T_eff than by using Ballasteros et al. Was meant for a 3D-model of the Orion Arm I use for "navigation" in my science fiction saga.

(That is based on the second HIPPARCOS reduction parallaxes, not GAIA. Yet.)

 

I just used spectral types mentioned in SIMBAD database. They are taken from various publications in astrophysical journals (explicitly mentioned in SIMBAD). settingspeshka

Yigor
Rigelianoid wrote:

Was meant for a 3D-model of the Orion Arm I use for "navigation" in my science fiction saga.

 

Is it published ? 😎

Rigelianoid
Yigor wrote:

Is it published ? 😎

No, that's a Blender model with some Python scripts to outline trajectories, intersection points etc.

But it's useful and good fun – seeing e.g. (our) Orion constellation's main stars from a spaceship (camera) 100 pc galactically outbound from Sol. happy.png

Yigor

The Orion Trapezium Cluster is very important as the closest stellar nursery, harboring also an intermediate-mass black hole 🌌:

https://en.wikipedia.org/wiki/Trapezium_Cluster

 

Yigor

What about your science fiction saga ?  Could U share it ? wink

Rigelianoid

I send you a link by PM.

Rigelianoid
Yigor wrote:

intermediate-mass black hole 🌌:

I still wonder how those beasts eat and especially when.

Let BH mergers be out of ansatz, assume the BH mass-quivalent is >> than that of the incoming matter and make it a one-body prob with a Kerr BH at the center. "Kerr" because Schwarzschild is a little theoretical, a run-of-the-mile collapsar does have angular momentum.

An incoming object now makes it through the event horizon in finite eigentime. That's well known, freshman stuff.  For an observer at asymptotically flat space however, it takes infinite time, thus it never happens.

I am aware that one can transform "away" the coordinate-singularity of an event horizon, but those singularity-free coords have very little to do with time as we know it as one – and special – leg of a tetrade.  

According to Gauss' theorem however, it does not matter for Wheeler's hairs as recorded by that outside observer whether the incoming mass is a little outside or inside the event horizon, an integral over a full sphere big enough yields the same pull and angular momentum in both cases. 

But the question remains when BH eat.