scholarly journals The Astrophysical Distance Scale. III. Distance to the Local Group Galaxy WLM Using Multiwavelength Observations of the Tip of the Red Giant Branch, Cepheids, and JAGB Stars

2021 ◽  
Vol 907 (2) ◽  
pp. 112
Author(s):  
Abigail J. Lee ◽  
Wendy L. Freedman ◽  
Barry F. Madore ◽  
Kayla A. Owens ◽  
Andrew J. Monson ◽  
...  
Keyword(s):  
Local Group ◽  
Distance Scale ◽  
Red Giant ◽  
Group Galaxy ◽  
Local Group Galaxy ◽  
Multiwavelength Observations

UGC-A86 - A local group galaxy candidate

1991 ◽  
Vol 101 ◽  
pp. 465 ◽  
Author(s):  
A. Saha ◽  
John G. Hoessel
Keyword(s):  
Local Group ◽  
Group Galaxy ◽  
Local Group Galaxy

Is LGS 2 a Local Group galaxy

1981 ◽  
Vol 93 ◽  
pp. 35 ◽  
Author(s):  
S. van den Bergh ◽  
R. Racine
Keyword(s):  
Local Group ◽  
Group Galaxy ◽  
Local Group Galaxy

XMM-Newton survey of the Local Group galaxy M 33 – catalogue results and global properties

2005 ◽  
Vol 1 (S230) ◽  
pp. 160-161
Author(s):  
Z. Misanovic ◽  
W. Pietsch ◽  
F. Haberl ◽  
M. Ehle ◽  
D. Hatzidimitriou ◽  
...  
Keyword(s):  
Local Group ◽  
Global Properties ◽  
Group Galaxy ◽  
Local Group Galaxy

scholarly journals XMM-Newton survey of the Local Group galaxy M 33

2004 ◽  
Vol 426 (1) ◽  
pp. 11-24 ◽  
Author(s):  
W. Pietsch ◽  
Z. Misanovic ◽  
F. Haberl ◽  
D. Hatzidimitriou ◽  
M. Ehle ◽  
...  
Keyword(s):  
Local Group ◽  
Group Galaxy ◽  
Local Group Galaxy

scholarly journals B-supergiants in IC1613: testing low-Z massive star physics and evolution

2016 ◽  
Vol 12 (S329) ◽  
pp. 389-389
Author(s):  
Inés Camacho ◽  
Miriam García ◽  
Miguel A. Urbaneja ◽  
Artemio Herrero
Keyword(s):  
Massive Star ◽  
Local Group ◽  
Uv Spectroscopy ◽  
Physical Parameters ◽  
Physical Processes ◽  
Life And Death ◽  
The Galaxy ◽  
Nearby Galaxies ◽  
Group Galaxy ◽  
Local Group Galaxy

AbstractThe physical processes taking place in massive stars during their life and death are highly dependent on the metallicity (Z) of their parent cloud. Observations of these stars in low-Z nearby galaxies are crucial to understand these processes. IC1613 is the nearest Local Group galaxy with ongoing star formation and O-abundance lower than the SMC, although UV spectroscopy suggests it is not so metal poor. We performed a spectral analysis of early B-type stars in the galaxy, obtaining physical parameters and abundances. Our results confirm the low O-abundance of IC1613.

New Cepheid distances to nearby galaxies based on BVRI CCD photometry. II - The local group galaxy M33

1991 ◽  
Vol 372 ◽  
pp. 455 ◽  
Author(s):  
Wendy L. Freedman ◽  
Christine D. Wilson ◽  
Barry F. Madore
Keyword(s):  
Local Group ◽  
Ccd Photometry ◽  
Nearby Galaxies ◽  
Group Galaxy ◽  
Local Group Galaxy

scholarly journals Chemical and Photometric Evolution of the Local Group Galaxy NGC 6822 in a Cosmological Context

2006 ◽  
Vol 644 (2) ◽  
pp. 924-939 ◽  
Author(s):  
Leticia Carigi ◽  
Pedro Colin ◽  
Manuel Peimbert
Keyword(s):  
Local Group ◽  
Cosmological Context ◽  
Ngc 6822 ◽  
Group Galaxy ◽  
Local Group Galaxy

scholarly journals The Araucaria Project: The Distance to the Local Group Galaxy WLM from Near‐Infrared Photometry of Cepheid Variables

2008 ◽  
Vol 683 (2) ◽  
pp. 611-619 ◽  
Author(s):  
Wolfgang Gieren ◽  
Grzegorz Pietrzyński ◽  
Olaf Szewczyk ◽  
Igor Soszyński ◽  
Fabio Bresolin ◽  
...  
Keyword(s):  
Near Infrared ◽  
Local Group ◽  
Infrared Photometry ◽  
Cepheid Variables ◽  
Group Galaxy ◽  
Local Group Galaxy

scholarly journals The Local Group Galaxy IC 1613 and its asymptotic giant branch variables

2015 ◽  
Vol 452 (1) ◽  
pp. 910-923 ◽  
Author(s):  
John W. Menzies ◽  
Patricia A. Whitelock ◽  
Michael W. Feast
Keyword(s):  
Local Group ◽  
Asymptotic Giant Branch ◽  
Group Galaxy ◽  
Local Group Galaxy
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