Upload
valmai
View
32
Download
0
Tags:
Embed Size (px)
DESCRIPTION
HD 37806 Slavek Rucinski Halifax 2010. Ae/Be Herbig star. In the Sigma Ori cluster field. Orion OB1b association. Young, moderately massive: 1.5 – 5 solar mass. A2Vpe. V ~ 7.95. M V ~ +0.2. ~350 pc (420 pc) HD 37806, known also as MWC 120 - PowerPoint PPT Presentation
Citation preview
1
HD 37806
Slavek Rucinski
Halifax 2010
2
Ae/Be Herbig star
In the Sigma Ori cluster field. Orion OB1b association.
Young, moderately massive: 1.5 – 5 solar mass.
A2Vpe. V ~ 7.95. MV ~ +0.2. ~350 pc (420 pc)
HD 37806, known also as MWC 120
One of first radio stars (Algonquin telescope 1973).
3
MOST light curve
4
MOST amplitude spectrum
5
ESO 1985 – 1986; ASAS 2001 - 2009
6
MOST data: Morlet-6 wavelet
7
MOST data: DOG-2 wavelet
8
MOST data: Scalegram (DOG-2 wavelet)
Stochastic self-similar noise process: X(λt) = λαX(t)
The slope implies α ≈ 1.5, same for cataclysmic binaries.
9
The paper
MNRAS: failure, insufficient interpretation and conclusions.
A&Ap: A good, positive review, but… - Expand on interpretation. - Explain why not pulsations, eclipses, spots. - Include Hp data? Use raw TYCHO, if available. - The star is a binary! Recent paper, MNRAS 2010