2012AJ....143...71K


Query : 2012AJ....143...71K

2012AJ....143...71K - Astron. J., 143, 71 (2012/March-0)

IRAS 03063+5735: a bowshock nebula powered by an early B star.

KOBULNICKY H.A., LUNDQUIST M.J., BHATTACHARJEE A. and KERTON C.R.

Abstract (from CDS):

Mid-infrared images from the Spitzer Space Telescope Galactic Legacy Infrared MidPlane Survey Extraordinaire program reveal that the infrared source IRAS 03063+5735 is a bowshock nebula produced by an early B star, 2MASS 03101044+5747035. We present new optical spectra of this star, classify it as a B1.5 V, and determine a probable association with a molecular cloud complex at VLSR= -38 to -42 km/s in the outer Galaxy near ℓ = 140°.59, b = -0°.250. On the basis of spectroscopic parallax, we estimate a distance of 4.0±1 kpc to both the bowshock nebula and the molecular complex. One plausible scenario is that this is a high-velocity runaway star impinging upon a molecular cloud. We identify the H II region and stellar cluster associated with IRAS 03064+5638 at a projected distance of 64 pc as one plausible birth site. The spectrophotometric distance and linkage to a molecular feature provides another piece of data helping to secure the ill-determined rotation curve in the outer Galaxy. As a by-product of spectral typing this star, we present empirical spectral diagnostic diagrams suitable for approximate spectral classification of O and B stars using He lines in the little-used yellow-red portion of the optical spectrum.

Abstract Copyright: ∼

Journal keyword(s): infrared: ISM - stars: early-type - stars: individual: 2MASS J03101044+5747035

CDS comments: p.4: #2 is [KGK2010] 2, #5 is [KGK2010] 5.

Simbad objects: 39

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Number of rows : 39
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 * 1 Per SB* 01 51 59.3200840608 +55 08 50.583693732 4.51 5.34 5.52     B1.5V 156 0
2 * eps Cas Be* 01 54 23.7340861680 +63 40 12.360238788 2.61 3.22 3.37 3.40 3.52 B3Vp_sh 207 0
3 * 11 Per * 02 43 02.8380253536 +55 06 21.666195864 5.13 5.639 5.753     B8IV 82 0
4 * lam Cet * 02 59 42.8925388548 +08 54 26.589196584 4.13 4.58 4.70 4.72 4.70 B6III 105 0
5 HD 18537 Pu* 03 00 52.2110264304 +52 21 06.248122308 4.78 5.158 5.219     B7V 87 0
6 * gam Per SB* 03 04 47.8201112829 +53 30 23.262605954 4.08 3.63 2.93 2.34 1.89 G9III+A2-III: 225 0
7 * bet Per SB* 03 08 10.1324535 +40 57 20.328013 1.70 2.07 2.12 2.08 2.11 B8V 1265 1
8 IRAS 03063+5735 IR 03 10 09.8525458368 +57 47 16.698344208           ~ 8 0
9 UCAC3 296-64470 * 03 10 10.4446180008 +57 47 03.621653700   16.37   15.80   B1.5V 2 0
10 [BDB2003] G141.08-01.06 Cl* 03 10 15 +56 50.3           ~ 3 0
11 IRAS 03064+5638 HII 03 10 15.3 +56 50 18           ~ 28 0
12 NGC 1220 OpC 03 11 40.6 +53 20 39     11.8     ~ 33 0
13 * 29 Per Pu* 03 18 37.7416927200 +50 13 19.834697676 6.232 5.074 5.157     B3V 167 0
14 * 31 Per Pu* 03 19 07.6392847536 +50 05 41.889763428 4.44 4.962 5.032     B5V 146 0
15 HD 21278 SB* 03 28 03.0707602272 +49 03 46.325803896   4.89 4.97     B5V 220 0
16 * 34 Per * 03 29 22.0494961351 +49 30 32.230623601 4.01 4.610 4.735     B3V 172 0
17 HD 21856 Pu* 03 32 40.0150232424 +35 27 42.207495156 4.96 5.807 5.900     B1V 192 0
18 * o Per * 03 42 22.6459308614 +33 57 54.093701142 4.13 4.912 4.972     B0.5V 315 0
19 * del Per Be* 03 42 55.4928046977 +47 47 14.988257477 2.38 2.89 3.01 2.99 3.10 B5III 328 0
20 * omi Per SB* 03 44 19.1337687984 +32 17 17.687367960 3.13 3.91 3.91 3.71 3.71 B1III 628 0
21 HD 23990 * 03 49 46.4941873182 +09 24 26.986474742 6.580 6.730 6.760     B9 27 0
22 HD 24131 * 03 51 53.7187356648 +34 21 32.823349956 4.96 5.730 5.772     B1V 183 0
23 HD 24504 * 03 55 58.1738380032 +47 52 17.123015028   5.297 5.379     B6V 80 0
24 * d Per bC* 04 21 33.1662438000 +46 29 55.964841936 4.31 4.757 4.812     B4IV 200 1
25 * 1 Cam ** 04 32 01.84227 +53 54 39.0450 6.41 5.876 5.772     B0III+B0IV/V 108 0
26 * nu. Eri bC* 04 36 19.1419185396 -03 21 08.857744927 2.82 3.737 3.928     B2III 407 0
27 * pi.04 Ori SB* 04 51 12.3657730111 +05 36 18.373859886 2.700 3.500 3.680 3.74 3.90 B2III 319 0
28 * pi.05 Ori SB* 04 54 15.0970445784 +02 26 26.417970456 2.72 3.54 3.73 3.79 3.99 B2III 225 0
29 * phi01 Ori Y*O 05 34 49.2376273598 +09 29 22.510380606 3.29 4.26 4.41 4.42 4.59 B0.2IV 272 0
30 RLP 545 LP* 20 32 03.7666533504 +41 25 10.443609084 15.15 14.76 13.24     B0.5V 25 0
31 RLP 619 SB* 20 32 19.6472111832 +41 20 38.899179780 14.79 14.53 13.25     B1.5V+B 18 0
32 2MASS J20323835+4128567 * 20 32 38.3435626200 +41 28 56.719109964   15.68 14.43     B3V 16 0
33 2MASS J20325667+4123408 * 20 32 56.6636273064 +41 23 40.890896304 15.41 15.09 13.81     B1V 19 0
34 Schulte 41 SB* 20 32 59.6317342392 +41 15 14.679727632 16.54 15.59 13.49     O9.7III(n) 37 0
35 RLP 678 EB* 20 33 10.5041613984 +41 22 22.405661292 14.97 14.54 12.958     B0V+(B3V+B6V) 44 0
36 Ass Cyg OB 2 As* 20 33.2 +41 19           ~ 1023 0
37 EM* AS 428 SB* 20 33 39.7935831360 +41 22 52.188298860 13.17 12.21 11.38     B1V+B1: 38 0
38 2MASS J20343455+4158295 * 20 34 34.5484020600 +41 58 29.656019316           OB 10 0
39 [CPR2002] A10 * 20 34 55.1114749680 +40 34 44.300082360           O9V 13 0

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