2018PASP..130k4302K

Query : 2018PASP..130k4302K

2018PASP..130k4302K - Publ. Astron. Soc. Pac., 130, part no 11, 4302-114302 (2018/November-0)

The Milky Way rotation curve revisited.

KRELOWSKI J., GALAZUTDINOV G. and STROBEL A.

Abstract (from CDS):

The paper revisits the problem described in detail in our Paper I (Galazutdinov et al.) concluding that the rotation curve of the thin gaseous Galactic disk, represented by the CaII lines, is Keplerian outside the solar orbit rather than flat. Now we apply new trigonometric Gaia parallaxes, published in the Data Release 2. We demonstrate that the distances, measured using Gaia parallaxes and CaII column densities, coincide statistically without systematic difference. Consequently, the result shown in Paper I is confirmed: the orbital motion of Galactic translucent clouds is not affected by hypothetical dark matter.

Abstract Copyright: © 2018. The Astronomical Society of the Pacific. All rights reserved.

Journal keyword(s):

Simbad objects: 48

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Number of rows : 48
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 * kap Cas s*b 00 32 59.9918836206 +62 55 54.413126128 3.50 4.30 4.16 4.02 3.96 BC0.7Ia 474 0
2 HD 12323 SB* 02 02 30.1268458032 +55 37 26.372271540 7.95 8.87 8.92     ON9.2V 193 0
3 * 5 Per s*b 02 11 29.1934233120 +57 38 43.964680956 6.23 6.68 6.35 6.02 5.75 B5Ia 191 0
4 HD 13256 s*b 02 11 43.9098216480 +60 42 44.500379976 9.8 9.69 8.68     B1Ia 71 0
5 HD 13716 EB* 02 15 39.4071948960 +57 45 47.947145364 8 8.53 8.30     B1.5Ib 79 0
6 HD 13758 Be* 02 16 04.4329318488 +57 44 41.675310168 8.85 9.39 9.14     B1V 55 0
7 BD+59 451 * 02 16 10.7764952472 +59 41 05.587971288 9.7 9.97 9.37     B1II 34 0
8 HD 13831 Pu* 02 16 39.2180538048 +56 44 16.085742396 7.56 8.32 8.26     O9.5I 83 1
9 HD 13841 s*b 02 16 46.3906698552 +57 01 45.670054584 6.95 7.60 7.37 7.11 6.95 B1.5Ib 132 0
10 HD 13854 s*b 02 16 51.7162480872 +57 03 18.882144756 6.10 6.76 6.48 6.14 5.95 B1Iab 217 0
11 HD 13866 Pu* 02 16 57.5756166480 +56 43 07.678553592 6.95 7.63 7.51     B2Ib-II:p 130 1
12 HD 13890 Be* 02 17 08.2163055288 +56 46 11.096889888 8.06 8.64 8.6370     B2.0III 74 0
13 HD 13969 * 02 17 49.8454024416 +57 05 25.578297996 8.56 9.15 8.0183 8.56 7.5970 B0.7III 76 0
14 HD 14014 bC* 02 18 00.0325766088 +56 13 57.341937648 8.23 8.95 8.86     B0.5V 43 0
15 BD+59 456 * 02 18 13.7667228240 +59 48 07.527109176 10.02 10.39 9.98     B0.5V 39 0
16 V* V757 Per bC* 02 18 23.0493577512 +57 00 36.728373708 8.05 8.67 7.8288 8.17 7.4510 B0.7II 88 0
17 * 61 And s*b 02 19 04.4525174952 +57 08 07.795069656 6.63 7.00 6.5678   6.6876 B3Ia 212 0
18 HD 14143 s*b 02 19 13.9420338600 +57 10 09.234950232 6.71 7.16 6.7000     B2Ia 208 0
19 HD 14302 * 02 20 34.1281186272 +56 19 47.839210032 8.27 8.81 8.64     B1II-III 47 0
20 HD 14357 bC* 02 21 10.4369424696 +56 51 56.340040320 8.31 8.83 8.4988 8.21 8.0630 B2.0I 82 0
21 HD 14434 Em* 02 21 52.4121560832 +56 54 18.032028876 7.87 8.65 8.49 8.29 8.20 O5.5Vnn((f))p 198 0
22 HD 14443 V* 02 22 00.5764087032 +57 08 41.872012908 7.85 8.39 7.6934 7.70 7.2734 BC2Ib 113 0
23 BD+56 574 V* 02 22 07.3838588088 +57 06 42.254596908 8.27 8.83 8.5330     B1III 58 0
24 V* V595 Per bC* 02 22 08.5707880560 +57 07 28.398038160 8.80 9.37 8.3166   7.7657 B0.5IV 59 0
25 HD 14442 V* 02 22 10.7004415512 +59 32 58.893287604 9.01 9.58 9.27     O5n(f)p 110 0
26 HD 14476 Pu* 02 22 16.9579243824 +57 16 18.963026868 8.62 9.13 8.1914   7.6376 B1.5I 55 0
27 V* DN Cas SB* 02 23 11.5401628296 +60 49 50.178378072 10.22 10.46 9.93     O8.5V 93 0
28 HD 236960 * 02 24 28.7776728456 +59 13 44.027886288 9.7 10.20 9.77     B1 31 0
29 * 10 Per s*b 02 25 16.0283450208 +56 36 35.354429280 5.95 6.56 6.26 5.93 5.74 B2Ia 248 0
30 BD+61 411 Y*O 02 26 34.3948 +62 00 42.380 11.09 11.14 10.28     O6.5V((f))z 63 0
31 HD 14947 s*b 02 26 46.9899705528 +58 52 33.118732380 7.83 8.44 7.98     O4.5If 262 0
32 BD+60 493 s*b 02 30 51.3556566000 +61 10 39.975724344 10.571 9.12 8.48     B0.5Iae 70 0
33 BD+60 498 Y*O 02 32 10.8542551368 +61 33 07.940208384 11.61 10.47 9.94     O9V 113 0
34 BD+60 499 Y*O 02 32 16.7518284696 +61 33 14.996422332 10.27 10.85 10.31     O9.5V 87 0
35 BD+60 501 Y*O 02 32 36.2781863760 +61 28 25.586191812 11.062 10.02 9.56     O7V(n)((f))z 124 0
36 HD 15558 Y*O 02 32 42.5366901168 +61 27 21.572901360 7.82 8.37 7.87 7.34 6.94 O4.5III(f) 324 0
37 HD 15570 Y*O 02 32 49.4207394600 +61 22 42.089384892 8.40 8.80 8.11 7.41 6.86 O4If 316 0
38 HD 15629 Y*O 02 33 20.5873992264 +61 31 18.188762844 8.23 8.85 8.42     O4.5V((fc)) 255 0
39 BD+60 513 Y*O 02 34 02.5297182912 +61 23 10.877763048 9.38 9.88 9.39     O7Vnz 116 0
40 HD 15785 s*b 02 34 48.0522508344 +60 33 07.449247908 10.033 8.82 8.37     B1Iab 82 0
41 BD+60 526 * 02 38 20.5920735960 +61 04 09.707000556 9.06 9.37 8.87     B2III: 28 0
42 HD 16310 * 02 39 23.0293856904 +59 03 59.451289416 10.026 8.64 8.10     B1II: 54 0
43 HD 16429 ** 02 40 44.9492589168 +61 16 55.995618720 7.91 8.29 7.67     O9.5III+F4V 165 1
44 BD+61 468 * 02 43 20.5813142496 +62 08 19.874547744   10.06 9.83     B2III: 17 0
45 HD 17505 ** 02 51 07.97514 +60 25 03.8720 6.83 7.47 7.07     O6.5III((f))n+O8V 205 0
46 HD 17520 ** 02 51 14.4527711976 +60 23 10.057239852 7.86 8.54 8.24 7.96 7.73 O9.2Ve+O8Vz 151 0
47 BD+60 594 * 02 57 04.1273587152 +61 24 57.669134904 10.563 9.58 9.30     O9.5IV-V 98 0
48 HD 20336 Be* 03 19 59.2693390128 +65 39 08.285606820 3.93 4.70 4.85 4.88 5.01 B2.5Vn(e) 226 0

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