2006A&A...454..781L


C.D.S. - SIMBAD4 rel 1.7 - 2021.04.16CEST14:27:31

2006A&A...454..781L - Astronomy and Astrophysics, volume 454, 781-796 (2006/8-2)

2MASS wide field extinction maps. I. The Pipe nebula.

LOMBARDI M., ALVES J. and LADA C.J.

Abstract (from CDS):

We present a 8°x6°, high resolution extinction map of the Pipe nebula using 4.5 million stars from the Two Micron All Sky Survey (2MASS) point source catalog. The use of Nicer (Lombardi & Alves, 2001A&A...377.1023L), a robust and optimal technique to map the dust column density, allows us to detect a AV=0.5mag extinction at a 3-σ level with a 1-arcmin resolution. (i) We find for the Pipe nebula a normal reddening law, E(J-H)=(1.85/-0.15)E(H-K). (ii) We measure the cloud distance using Hipparchos and Tycho parallaxes, and obtain 130+24–58pc. This, together with the total estimated mass, 104M, makes the Pipe the closest massive cloud complex to Earth. (iii) We compare the Nicer extinction map to the NANTEN 12CO observations and derive with unprecedented accuracy the relationship between the near-infrared extinction and the 12CO column density and hence (indirectly) the 12CO X-factor, that we estimate to be 2.91x1020/cm2/K/km/s in the range AV ∈[0.9, 5.4]mag. (iv) We identify approximately 1500 OH/IR stars located within the Galactic bulge in the direction of the Pipe field. This represents a significant increase of the known numbers of such stars in the Galaxy. Our analysis confirms the power and simplicity of the color excess technique to study molecular clouds. The comparison with the NANTEN 12CO data corroborates the insensitivity of CO observations to low column densities (up to approximately 2mag in AV), and shows also an irreducible uncertainty in the dust-CO correlation of about 1mag of visual extinction.

Abstract Copyright:

Journal keyword(s): ISM: clouds - ISM: dust, extinction - ISM: structure - ISM: individual objects: Pipe molecular complex - methods: data analysis

Simbad objects: 9

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Number of rows : 9

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
#notes
1 NAME Taurus Complex SFR 04 41.0 +25 52           ~ 3679 0
2 NAME Lup Cloud SFR 16 03 -38.1           ~ 558 0
3 NAME Ophiuchus Molecular Cloud SFR 16 28 06 -24 32.5           ~ 3156 1
4 LDN 1746 DNe 17 11.3 -27 22           ~ 117 0
5 [RNC96] B59-MMS 1 mm 17 11 22.1 -27 24 28           ~ 6 0
6 HD 158233 PM* 17 29 06.5561989448 -23 50 10.003820210 12.053 10.904 9.597 8.798 8.111 K5V 32 0
7 NAME the Pipe Nebula DNe 17 30 -25.0           ~ 351 1
8 IC 5146 OpC 21 53 24 +47 16.0           ~ 400 2
9 NAME Galactic Bulge reg ~ ~           ~ 3564 0

    Equat.    Gal    SGal    Ecl

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2021.04.16-14:27:31

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