Sign on
ADS Classic is now deprecated. It will be completely retired in October 2019. This page will automatically redirect to the new ADS interface at that point.

SAO/NASA ADS Astronomy Abstract Service


· Find Similar Abstracts (with default settings below)
· Electronic On-line Article (HTML)
· Table of Contents
· References in the Article
· Citations to the Article (1) (Citation History)
· Refereed Citations to the Article
· Also-Read Articles (Reads History)
·
· Translate This Page
Title:
The structure of the ISM in the Zone of Avoidance by high-resolution multi-wavelength observations
Authors:
Tóth, L. V.; Doi, Y.; Pinter, S.; Kovács, T.; Zahorecz, S.; Bagoly, Z.; Balázs, L. G.; Horvath, I.; Racz, I. I.; Onishi, T.
Affiliation:
AA(Eötvös University, Budapest, ; MTA CSFK Konkoly Observatory, Budapest), AB(Department of Earth Science and Astronomy, The University of Tokyo, 3-8-1 Komaba, Meguro-ku, Tokyo 153-8902, Japan), AC(Eötvös University, Budapest), AD(Eötvös University, Budapest), AE(Osaka Prefecture University, 1-1 Gakuen-cho, Naka-ku, Sakai, Osaka 599-8531, Japan; Chile Observatory, NAOJ, NINS, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan), AF(Eötvös University, Budapest), AG(Eötvös University, Budapest; MTA CSFK Konkoly Observatory, Budapest), AH(National University of Public Service, Budapest), AI(Eötvös University, Budapest; MTA CSFK Konkoly Observatory, Budapest), AJ(Osaka Prefecture University, 1-1 Gakuen-cho, Naka-ku, Sakai, Osaka 599-8531, Japan)
Publication:
Peering towards Cosmic Dawn, Proceedings of the International Astronomical Union, IAU Symposium, Volume 333, pp. 162-165
Publication Date:
05/2018
Origin:
CUP
Keywords:
ISM: structure, infrared: ISM, gamma-ray burst: general, GRB110213A
Abstract Copyright:
(c) 2018: Copyright © International Astronomical Union 2018
DOI:
10.1017/S1743921317011541
Bibliographic Code:
2018IAUS..333..162T

Abstract

We estimate the column density of the Galactic foreground interstellar medium (GFISM) in the direction of extragalactic sources. All-sky AKARI FIS infrared sky survey data might be used to trace the GFISM with a resolution of 2 arcminutes. The AKARI based GFISM hydrogen column density estimates are compared with similar quantities based on HI 21cm measurements of various resolution and of Planck results. High spatial resolution observations of the GFISM may be important recalculating the physical parameters of gamma-ray burst (GRB) host galaxies using the updated foreground parameters.
Bibtex entry for this abstract   Preferred format for this abstract (see Preferences)


Find Similar Abstracts:

Use: Authors
Title
Keywords (in text query field)
Abstract Text
Return: Query Results Return    items starting with number
Query Form
Database: Astronomy
Physics
arXiv e-prints