SIMBAD references

2018ApJ...858..111R - Astrophys. J., 858, 111-111 (2018/May-2)

The connection between different tracers of the diffuse interstellar medium: kinematics.

RICE J.S., FEDERMAN S.R., FLAGEY N., GOLDSMITH P.F., LANGER W.D., PINEDA J.L. and LAMBERT D.L.

Abstract (from CDS):

Using visible, radio, microwave, and submillimeter data, we study several lines of sight toward stars generally closer than 1 kpc on a component-by-component basis. We derive the component structure seen in absorption at visible wavelengths from Ca II, Ca I, K I, CH, CH+, and CN and compare it to emission from H I, CO and its isotopologues, and C+ from the GOT C+ survey. The correspondence between components in emission and absorption helps create a more unified picture of diffuse atomic and molecular gas in the interstellar medium. We also discuss how these tracers are related to the CO-dark H2 gas probed by C+ emission and discuss the kinematic connections among the species observed.

Abstract Copyright: © 2018. The American Astronomical Society. All rights reserved.

Journal keyword(s): ISM: atoms - ISM: clouds - ISM: molecules - ISM: structure - radio lines: ISM - submillimeter: ISM

VizieR on-line data: <Available at CDS (J/ApJ/858/111): table1.dat table2.dat>

Simbad objects: 31

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