Display data from paper

Select data type:

NII11 - Astrometry of H₂O Masers in the Massive Star-Forming Region IRAS 06061+2151 with VERA

Interferometry data

Short title: Niinuma et al. (2011)
Authors: Niinuma, KotaroNagayama, TakumiHirota, TomoyaHonma, MarekiMotogi, KazuhitoNakagawa, AkiharuKurayama, TomoharuKan-Ya, YukitoshiKawaguchi, NoriyukiKobayashi, HideyukiUeno, Yuji
Journal: Publications of the Astronomical Society of Japan, Vol.63, No.1, pp.9--16
Bibcode:

Target type: High_mass_SFR

Abstract
We measured the trigonometric annual parallax of an H2O maser source associated with the massive star-forming region IRAS 06061+2151 with VERA. The annual parallax of 0.496�0.031 mas, corresponding to a distance of 2.02+0.13-0.12kpc, was obtained by 10 epochs of observations during the period from 2007 October to 2009 September. This distance was obtained more accurately than the photometric one previously measured, and places IRAS 06061+2151 in the Perseus spiral arm. We found that IRAS 06061+2151 also has a peculiar motion of larger than 15 km s-1 which is counter to the Galactic rotation. This is similar to the motions of five sources in the Perseus spiral arm, whose parallaxes and proper motions have already been measured with satisfactory accuracy. Moreover, these sources move with an average of 27 km s-1 toward the Galactic center and counter to the Galactic rotation.

Abstract

We measured the trigonometric annual parallax of an H2O maser source associated with the massive star-forming region IRAS 06061+2151 with VERA. The annual parallax of 0.496�0.031 mas, corresponding to a distance of 2.02+0.13-0.12kpc, was obtained by 10 epochs of observations during the period from 2007 October to 2009 September. This distance was obtained more accurately than the photometric one previously measured, and places IRAS 06061+2151 in the Perseus spiral arm. We found that IRAS 06061+2151 also has a peculiar motion of larger than 15 km s-1 which is counter to the Galactic rotation. This is similar to the motions of five sources in the Perseus spiral arm, whose parallaxes and proper motions have already been measured with satisfactory accuracy. Moreover, these sources move with an average of 27 km s-1 toward the Galactic center and counter to the Galactic rotation.

Download as: Table (CSV)
View as list of objects

Detection table from Niinuma et al. (2011)

Export table to csv

Hide / Show individual components

ID	Obs. RA	Obs. Dec	RA offset	Dec offset	l	b	Group id	#	Maser spot	Source name	Image	Descr.	Line	V_peak	μ_X	μ_Y	π	Telescope	Detection	Class	Dist. (parallax)	Date
	(J2000)	(J2000)	(mas)	(mas)	(deg.)	(deg.)							H₂O	(km/s)	(mas/yr)	(mas/yr)	(mas)		Yes/No		(kpc)
1	+06 09 6.970593	+21 50 41.204897			188.7937343	1.0306213	G188.796+1.033			IRAS 06061+2151	Image	Descr	22 GHz;	-8				VERA	+H₂O -CH₃OH I +CH₃OH II -OH	SFR	2.02 (+0.13 -0.12)	2007 Oct - 2009 Sep
	+06 09 6.97056233	+21 50 41.20472	-0.325 mas	-0.04 mas	188.793734	1.030621		1	1	IRAS 06061+2151				-9.48	0.11 (0.12)	-4.04 (0.10)	0.518 (0.084)
	+06 09 6.97056607	+21 50 41.204706	-0.269 mas	-0.054 mas	188.793734	1.030621		2	2	IRAS 06061+2151				-9.269	-0.07 (0.15)	-3.88 (0.12)	0.539 (0.119)
	+06 09 6.9705726	+21 50 41.204715	-0.171 mas	-0.045 mas	188.793734	1.030621		3	3	IRAS 06061+2151				-9.059	-0.01 (0.14)	-3.88 (0.13)	0.533 (0.114)
	+06 09 6.9705786	+21 50 41.204728	-0.081 mas	-0.032 mas	188.793734	1.030621		4	4	IRAS 06061+2151				-8.848	-0.14 (0.13)	-3.88 (0.13)	0.522 (0.102)
	+06 09 6.9705818	+21 50 41.204748	-0.033 mas	-0.012 mas	188.793734	1.030621		5	5	IRAS 06061+2151				-8.637	-0.19 (0.13)	-3.89 (0.12)	0.495 (0.103)
	+06 09 6.97058393	+21 50 41.204755	-0.001 mas	-0.005 mas	188.793734	1.030621		6	6	IRAS 06061+2151				-8.427	-0.21 (0.14)	-3.90 (0.12)	0.481 (0.110)
	+06 09 6.9705856	+21 50 41.204773	0.024 mas	0.013 mas	188.793734	1.030621		7	7	IRAS 06061+2151				-8.216	-0.20 (0.14)	-3.92 (0.11)	0.473 (0.111)
	+06 09 6.97058727	+21 50 41.204785	0.049 mas	0.025 mas	188.793734	1.030621		8	8	IRAS 06061+2151				-8.005	-0.14 (0.13)	-3.92 (0.10)	0.466 (0.103)
	+06 09 6.97058733	+21 50 41.20482	0.05 mas	0.06 mas	188.793734	1.030621		9	9	IRAS 06061+2151				-7.795	-0.07 (0.18)	-4.01 (0.12)	0.416 (0.116)
	+06 09 6.9705916	+21 50 41.204879	0.114 mas	0.119 mas	188.793734	1.030621		10	10	IRAS 06061+2151				-7.584	-0.05 (0.27)	-3.92 (0.18)	0.419 (0.137)
	+06 09 6.971813	+21 50 41.217094	18.435 mas	12.334 mas	188.793734	1.030627		11	11	IRAS 06061+2151				-7.373	-0.12 (0.12)	-3.75 (0.19)	0.641 (0.120)

DSS colored	2MASS colored	WISE colored
SDSS color	IRAC color I1,I2,I4	GLIMPSE 360
PACS color (70-160 um)	SPIRE color (250-500 um)	NVSS (1.4GHz)
ATLASGAL 870 um	ATLASGAL 870 um + Planck	Bolocam 1.1 mm
UKIDSS K Download UKIDSS K FITS	2MASS K Download 2MASS K FITS

select MAX(h2o_data_all.ra_hms) as ra_hms,MAX(h2o_data_all.dec_dms) as dec_dms,MAX(h2o_data_all.source_name) as source_name,MAX(h2o_data_all.ra) as ra,MAX(h2o_data_all.dec) as dec,MAX(h2o_data_all.l) as l,MAX(h2o_data_all.b) as b,MAX(h2o_data_all.grp) as grp,MAX(h2o_data_all.other_name) as other_name,MAX(h2o_data_all.other_desc) as other_desc,BOOL_OR(thermal) as thermal,MAX(h2o_data_all.line) as line,MAX(h2o_data_all.vrange) as vrange,MAX(h2o_data_all.vpeak) as vpeak,MAX(h2o_data_all.peak) as peak,MAX(h2o_data_all.fwhm) as fwhm,MAX(h2o_data_all.int) as int,MAX(h2o_data_all.rms) as rms,MAX(h2o_data_all.units) as units,MAX(h2o_data_all.units_rms) as units_rms,MAX(h2o_data_all.date_txt) as date_txt,MAX(h2o_data_all.telescope_ref) as telescope_ref,MAX(h2o_data_all.telescope_conf) as telescope_conf,MAX(h2o_data_all.v_step) as v_step,MAX(h2o_data_all.beam) as beam,MAX(h2o_data_all.beam_maj) as beam_maj,MAX(h2o_data_all.beam_min) as beam_min,MAX(h2o_data_all.beam_pa) as beam_pa,MAX(h2o_data_all.ref) as ref,MAX(h2o_data_all.list_ref) as list_ref,MAX(h2o_data_all.ascii) as ascii,MAX(h2o_data_all.url) as url,MAX(h2o_data_all.image) as image,MAX(h2o_data_all.image2) as image2,MAX(h2o_data_all.image3) as image3,MAX(h2o_data_all.descr) as descr,MAX(h2o_data_all.id) as id,BOOL_OR(mjy_flag) as mjy_flag,BOOL_OR(rms_mjy_flag) as rms_mjy_flag,MAX(h2o_data_all.dist) as dist,1 as dist_parallax,MAX(h2o_data_all.date_txt) as date_txt,MAX(line_det) as line_det,MAX(type) as type,MAX(simbad_types_cat) as simbad_types_cat FROM h2o_data_all  LEFT JOIN all_objects_withmet ON h2o_data_all.grp=all_objects_withmet.group_name LEFT JOIN object_categories ON all_objects_withmet.group_name = object_categories.group_name_cat AND object_categories.tbl_cat = 'all_objects_withmet' LEFT JOIN transitions ON h2o_data_all.line=transitions."Line"  WHERE ref ilike 'NII11' AND detected=true AND hide=false GROUP BY ref

select h2o_data_all.ra_hms,h2o_data_all.dec_dms,h2o_data_all.source_name,h2o_data_all.ra,h2o_data_all.dec,h2o_data_all.l,h2o_data_all.b,h2o_data_all.grp,h2o_data_all.other_name,h2o_data_all.other_desc,h2o_data_all.thermal,h2o_data_all.line,h2o_data_all.vrange,h2o_data_all.vpeak,h2o_data_all.peak,h2o_data_all.fwhm,h2o_data_all.int,h2o_data_all.rms,h2o_data_all.units,h2o_data_all.units_rms,h2o_data_all.date_txt,h2o_data_all.telescope_ref,h2o_data_all.telescope_conf,h2o_data_all.v_step,h2o_data_all.beam,h2o_data_all.beam_maj,h2o_data_all.beam_min,h2o_data_all.beam_pa,h2o_data_all.ref,h2o_data_all.list_ref,h2o_data_all.ascii,h2o_data_all.url,h2o_data_all.image,h2o_data_all.image2,h2o_data_all.image3,h2o_data_all.descr,h2o_data_all.id,h2o_data_all.mjy_flag,h2o_data_all.rms_mjy_flag,h2o_data_all.dist,h2o_data_all.dist_parallax,h2o_data_all.date_txt,line_det,type,simbad_types_cat FROM h2o_data_all   LEFT JOIN all_objects_withmet ON h2o_data_all.grp=all_objects_withmet.group_name LEFT JOIN object_categories ON all_objects_withmet.group_name = object_categories.group_name_cat AND object_categories.tbl_cat = 'all_objects_withmet' LEFT JOIN transitions ON h2o_data_all.line=transitions."Line"  WHERE ref ilike 'NII11' AND detected=true AND hide=false ORDER BY detected DESC,id

Display data from paper

NII11 - Astrometry of H2O Masers in the Massive Star-Forming Region IRAS 06061+2151 with VERA

Interferometry data

View as list of objects

Detection table from Niinuma et al. (2011)

NII11 - Astrometry of H₂O Masers in the Massive Star-Forming Region IRAS 06061+2151 with VERA