output
19952026
most citedTrigonometric Parallaxes of High Mass Star Forming Regions: the Structure and Kinematics of the Milky Way

1.4k citations

Showing 2010 · astro-ph.GAShow all

15 papers · 2 filters

astro-ph.GA2010★ 21 cited

Centrosymmetric molecules as possible carriers of diffuse interstellar bands

M. Kazmierczak, M. R. Schmidt, G. A. Galazutdinov +3

In this paper, we present new data with interstellar C2 (Phillips bands A-X), from observations made with the Ultraviolet-Visual Echelle Spectrograph of the European Southern Obser…

astro-ph.GA2010★ 23 cited

Excitation temperature of C2 and broadening of the 6196A diffuse interstellar band

M. Kazmierczak, P. Gnacinski, M. R. Schmidt +3

This paper presents a finding of the correlation between the width of a strong diffuse interstellar band at 6196A and the excitation temperature of C2 based on high resolution and…

astro-ph.GA2010★ 30 cited

Abundances and rotational temperatures of the C2 interstellar molecule towards six reddened early-type stars

M. Kazmierczak, M. R. Schmidt, A. Bondar +1

Using high-resolution (~85000) and high signal-to-noise ratio (~200) optical spectra acquired with the European Southern Observatory Ultraviolet and Visual Echelle Spectrograph, we…

astro-ph.GA2010★ 18 cited

VLA observations of water masers towards 6.7 GHz methanol maser sources

A. Bartkiewicz, M. Szymczak, Y. M. Pihlström +3

22 GHz water and 6.7 GHz methanol masers are usually thought as signposts of early stages of high-mass star formation but little is known about their associations and the physical…

astro-ph.GA2010★ 48 cited

Detection of OH and HO towards Orion~KL

H. Gupta, P. Rimmer, J. C. Pearson +76

We report observations of the reactive molecular ions OH, HO, and HO towards Orion KL with Herschel/HIFI. All three fine-structure transitions of OH…

astro-ph.GA2010★ 16 cited

Herschel observations of deuterated water towards Sgr B2(M)

Claudia Comito, Peter Schilke, Rainer Rolffs +53

Observations of HDO are an important complement for studies of water, because they give strong constraints on the formation processes -- grain surfaces versus energetic process in…