The H II region luminosity function of the Milky Way

1989 ◽  
Vol 101 ◽  
pp. 649 ◽  
Author(s):  
Toby R. Smith ◽  
Robert C., Jr. Kennicutt
Keyword(s):  
Luminosity Function ◽  
Milky Way ◽  
H Ii Region

scholarly journals The Luminosity Function of the Milky Way Satellites

2008 ◽  
Vol 686 (1) ◽  
pp. 279-291 ◽  
Author(s):  
S. Koposov ◽  
V. Belokurov ◽  
N. W. Evans ◽  
P. C. Hewett ◽  
M. J. Irwin ◽  
...  
Keyword(s):  
Luminosity Function ◽  
Milky Way

scholarly journals H II REGION LUMINOSITY FUNCTION OF THE INTERACTING GALAXY M51

2011 ◽  
Vol 735 (2) ◽  
pp. 75 ◽  
Author(s):  
Jong Hwan Lee ◽  
Narae Hwang ◽  
Myung Gyoon Lee
Keyword(s):  
Luminosity Function ◽  
H Ii Region

scholarly journals The Galactic H ii Region Luminosity Function at Radio and Infrared Wavelengths

2021 ◽  
Vol 910 (2) ◽  
pp. 159
Author(s):  
J. L. Mascoop ◽  
L. D. Anderson ◽  
Trey. V. Wenger ◽  
Z. Makai ◽  
W. P. Armentrout ◽  
...  
Keyword(s):  
Luminosity Function ◽  
H Ii Region ◽  
Infrared Wavelengths

scholarly journals H II REGION METALLICITY DISTRIBUTION IN THE MILKY WAY DISK

2011 ◽  
Vol 738 (1) ◽  
pp. 27 ◽  
Author(s):  
Dana S. Balser ◽  
Robert T. Rood ◽  
T. M. Bania ◽  
L. D. Anderson
Keyword(s):  
Milky Way ◽  
H Ii Region ◽  
Metallicity Distribution

scholarly journals Luminosity function and radial distribution of Milky Way satellites in a ΛCDM Universe

2010 ◽  
Vol 402 (3) ◽  
pp. 1995-2008 ◽  
Author(s):  
Andrea V. Macciò ◽  
Xi Kang ◽  
Fabio Fontanot ◽  
Rachel S. Somerville ◽  
Sergey Koposov ◽  
...  
Keyword(s):  
Radial Distribution ◽  
Luminosity Function ◽  
Milky Way

scholarly journals OB ASSOCIATIONS AT THE UPPER END OF THE MILKY WAY LUMINOSITY FUNCTION

2013 ◽  
Vol 766 (2) ◽  
pp. 135 ◽  
Author(s):  
Mubdi Rahman ◽  
Christopher D. Matzner ◽  
Dae-Sik Moon
Keyword(s):  
Luminosity Function ◽  
Milky Way ◽  
Ob Associations

The H II region luminosity function of M51

1992 ◽  
Vol 103 ◽  
pp. 815 ◽  
Author(s):  
Richard J. Rand
Keyword(s):  
Luminosity Function ◽  
H Ii Region

scholarly journals Globular Cluster Systems: Comparison with the Milky Way

2002 ◽  
Vol 207 ◽  
pp. 68-72
Author(s):  
Dante Minniti
Keyword(s):  
Globular Cluster ◽  
Reference Point ◽  
Luminosity Function ◽  
Milky Way ◽  
Elliptical Galaxy ◽  
Cluster System ◽  
Cluster Systems ◽  
Distant Galaxies ◽  
Globular Cluster System

The Milky Way globular cluster system serves as a reference for the study of more distant galaxies. Here I stress that there are still things we do not know about the globular cluster system of our own galaxy: their total number, their spatial motions and distances, and their IR properties. If our best reference point is not fully known, caution should be exercised when interpreting observations of distant systems. At the same time, when studying distant ellipticals it is not always advisable to rely on the Milky Way as a comparison. For example, only recently the first full calibration of the luminosity function of the globular cluster system of an elliptical galaxy was made, necessary to compare apples with apples.

scholarly journals Hamburg Observatory Northern Milky Way Spectral Survey For Emission Objects

1984 ◽  
Vol 78 ◽  
pp. 311-314
Author(s):  
L. Kohoutek
Keyword(s):  
Emission Line ◽  
Milky Way ◽  
Planetary Nebulae ◽  
H Ii Region ◽  
Objective Prism ◽  
Protoplanetary Nebula ◽  
Spectral Survey ◽  
Individual Objects

Objective-prism spectral surveys open the possibility to search for faint emission-line objects with the aim to complete their statistics and to pick out most interesting individual objects for further study. In the years 1964 - 1970 the Hamburg Hα Spectral Survey of the Northern Milky Way was accomplished using the Schmidt camera (80/120 cm, f= 240 cm) in Bergedorf with the following parameters: area 1 32° - 214°, -10°<b<+10°, 160 fields. Kodak 103aE + RG1, exp. 60min, widen. 10", 4° prism (580 Å/mm at Hγ ). As a main result the list of about 140 faint objects classified as planetary nebulae or possible planetary nebulae (Kohoutek,1965, 1969a,1972), and the identification of about 1500 new stars having Hα in emission (Kohoutek, Wehmeyer, in preparation) can be reported. The best known examples of this survey are K 3-50, a prototype of a compact H II region, and the symbiotic variable HBV 475 = V 1329 Cyg (Kohoutek, 1969b), which is also classified as a protoplanetary nebula.

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