MID-INFRARED EXTINCTION AND ITS VARIATION WITH GALACTIC LONGITUDE

نویسندگان
چکیده

برای دانلود باید عضویت طلایی داشته باشید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Mid-Infrared Spectroscopic Diagnostics of Galactic Nuclei

In this paper I summarize the science motivations, as well as a few mid-infrared spectroscopic methods used to identify the principal mechanisms of energy production in dust enshrouded galactic nuclei. The development of the various techniques is briefly discussed. Emphasis is given to the use of the data which are becoming available with the infrared spectrograph (IRS) on Spitzer, as well as t...

متن کامل

Interstellar extinction in the open clusters towards galactic longitude around 130

In this paper we present a detailed study of the intra-cluster reddening material in the young open clusters located around l ∼ 130 using colour-excess diagrams and two-colour diagrams. The study supports the universality of the extinction curves for λ ≥ λJ , whereas for shorter wavelengths the curve depends upon the value of the Rcluster (total-to-selective absorption in the cluster region). T...

متن کامل

Probing ice clouds by mid-infrared extinction spectroscopy

Series of infrared extinction spectra of ice crystals were recorded in the 6000–800 cm −1 wavenumber regime during expansion cooling experiments in the large aerosol and cloud chamber AIDA of Forschungszentrum Karlsruhe. Either supercooled sulphuric acid solution droplets or dry mineral dust particles were added as seed aerosols to 5 initiate ice formation after having established ice supersatu...

متن کامل

The Galactic Extinction Toward GRB 970228 and Its Implications

The IRAS 100 micron image of the GRB 970228 field shows that the amount of galactic dust in this direction is substantial and varies on arcminute angular scales. From an analysis of the observed surface density of galaxies in the 2.6×2.6 HST WFPC image of the GRB 970228 field, we find AV = 1.1±0.10. From an analysis of the observed spectra of three stars in the GRB 970228 field, we find AV = 1....

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: The Astrophysical Journal

سال: 2009

ISSN: 0004-637X,1538-4357

DOI: 10.1088/0004-637x/707/1/89