Galactic Plane H Surveys: IPHAS & VPHAS+
arXiv:1507.02281 · doi:10.1007/978-3-319-19330-4_7
Abstract
The optical Galactic Plane H surveys IPHAS and VPHAS+ are dramatically improving our understanding of Galactic stellar populations and stellar evolution by providing large samples of stars in short lived, but important, evolutionary phases, and high quality homogeneous photometry and images over the entire Galactic Plane. Here I summarise some of the contributions these surveys have already made to our understanding of a number of key areas of stellar and Galactic astronomy.
5 pages, 2 figures, refereed proceeding of the "The Universe of Digital Sky Surveys" conference, November 2014, to be published in the Astrophysics and Space Science Proceedings
References in corpus (11)
- The VST Photometric Halpha Survey of the Southern Galactic Plane and Bulge (VPHAS+)
- The Second Data Release of the INT Photometric H-Alpha Survey of the Northern Galactic Plane (IPHAS DR2)
- The IPHAS Catalogue of Halpha Emission Line Sources in the Northern Galactic Plane
- A 3D extinction map of the Northern Galactic Plane based on IPHAS photometry
- A planetary nebula around nova V458 Vul undergoing flash ionization
- First release of the IPHAS Catalogue of New Extended Planetary Nebulae
- IPHAS discoveries of young stars towards Cyg OB2 and its southern periphery
- New OB star candidates in the Carina Arm around Westerlund 2 from VPHAS+
- The Ionized Nebula surrounding the Red Supergiant W26 in Westerlund 1
- Extremely red stellar objects revealed by IPHAS
- A determination of the space density and birth rate of hydrogen-line (DA) white dwarfs in the Galactic Plane, based on the UVEX survey