Abstract
Extragalactic surveys in the emission line of [O iii] λ 5007 have provided us with the absolute line strengths of large, homogeneous sets of planetary nebulae. These data have been used to address a host of problems, from the measurement of the extragalactic distance scale, to the study of stellar populations. I review our current understanding of the [O iii] planetary nebula luminosity function (PNLF), and discuss some of the physical processes that effect its structure. I also describe the features of the H PNLF, a function that, upon first glance, looks similar to the [O iii] PNLF, but which includes a very different set of objects. Finally, I discuss recent measurements of α, the number of PNe found in a stellar population, normalized to that population's bolometric luminosity. I show that, contrary to expectations, the values of found in actively star-forming spirals are essentially the same as those measured in late-type elliptical and lenticular systems. I discuss how this result sheds light on the physics of the planetary nebula phenomenon.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 149-155 |
| Number of pages | 7 |
| Journal | Publications of the Astronomical Society of Australia |
| Volume | 27 |
| Issue number | 2 |
| DOIs | |
| State | Published - Jun 10 2010 |
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All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science
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The Planetary Nebula Luminosity Function : Pieces of the Puzzle. / Ciardullo, Robin Bruce.
In: Publications of the Astronomical Society of Australia, Vol. 27, No. 2, 10.06.2010, p. 149-155.Research output: Contribution to journal › Article
TY - JOUR
T1 - The Planetary Nebula Luminosity Function
T2 - Pieces of the Puzzle
AU - Ciardullo, Robin Bruce
PY - 2010/6/10
Y1 - 2010/6/10
N2 - Extragalactic surveys in the emission line of [O iii] λ 5007 have provided us with the absolute line strengths of large, homogeneous sets of planetary nebulae. These data have been used to address a host of problems, from the measurement of the extragalactic distance scale, to the study of stellar populations. I review our current understanding of the [O iii] planetary nebula luminosity function (PNLF), and discuss some of the physical processes that effect its structure. I also describe the features of the H PNLF, a function that, upon first glance, looks similar to the [O iii] PNLF, but which includes a very different set of objects. Finally, I discuss recent measurements of α, the number of PNe found in a stellar population, normalized to that population's bolometric luminosity. I show that, contrary to expectations, the values of found in actively star-forming spirals are essentially the same as those measured in late-type elliptical and lenticular systems. I discuss how this result sheds light on the physics of the planetary nebula phenomenon.
AB - Extragalactic surveys in the emission line of [O iii] λ 5007 have provided us with the absolute line strengths of large, homogeneous sets of planetary nebulae. These data have been used to address a host of problems, from the measurement of the extragalactic distance scale, to the study of stellar populations. I review our current understanding of the [O iii] planetary nebula luminosity function (PNLF), and discuss some of the physical processes that effect its structure. I also describe the features of the H PNLF, a function that, upon first glance, looks similar to the [O iii] PNLF, but which includes a very different set of objects. Finally, I discuss recent measurements of α, the number of PNe found in a stellar population, normalized to that population's bolometric luminosity. I show that, contrary to expectations, the values of found in actively star-forming spirals are essentially the same as those measured in late-type elliptical and lenticular systems. I discuss how this result sheds light on the physics of the planetary nebula phenomenon.
UR - http://www.scopus.com/inward/record.url?scp=77953164125&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=77953164125&partnerID=8YFLogxK
U2 - 10.1071/AS09022
DO - 10.1071/AS09022
M3 - Article
VL - 27
SP - 149
EP - 155
JO - Publications of the Astronomical Society of Australia
JF - Publications of the Astronomical Society of Australia
SN - 1448-6083
IS - 2
ER -