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A new photometric study of Herbig Ae/Be stars in the infrared
DOI: 10.1016/j.newast.2015.09.001 Bibcode: 2016NewA...44....1C

Zhang, P.; Chen, P. S.; Shan, H. G.

In this paper we collected almost all HAeBe stars known so far (253 sources in total) to photometrically study their infrared properties. The 2MASS, WISE, IRAS and AKARI data are employed to make analyses. It is shown from several two-color diagrams that from 1 µm to 60 µm infrared radiations from circumstellar disks with the power law…

2016 New Astronomy
AKARI 30
The curious temporal behavior of the frequency of different class flares
DOI: 10.1016/j.newast.2015.08.004 Bibcode: 2016NewA...43...91G

Zhong, J.; Gao, P. X.

We investigate the frequency of all (X-ray flare events higher than class B1.0), B, C, M and X-class flares, respectively, derived from the National Geophysical Data Center (NGDC) list of solar flares between May 1983 and September 2014, which corresponds to the two complete solar cycles (SCs) 22 and 23 as well as the rise and maximum phases of SC…

2016 New Astronomy
Hinode 20
Flux and spectral variability of the blazar PKS 2155 -304 with XMM-Newton: Evidence of particle acceleration and synchrotron cooling
DOI: 10.1016/j.newast.2015.08.005 Bibcode: 2016NewA...44...21B

Bhagwan, Jai; Papadakis, I. E.; Wiita, Paul J. +1 more

We have analyzed XMM-Newton observations of the high energy peaked blazar, PKS 2155 -304, made on 24 May 2002 in the 0.3-10 keV X-ray band. These observations display a mini-flare, a nearly constant flux period and a strong flux increase. We performed a time-resolved spectral study of the data, by dividing the data into eight segments. We fitted t…

2016 New Astronomy
XMM-Newton 17
Detection of coronal mass ejections using AdaBoost on grayscale statistic features
DOI: 10.1016/j.newast.2016.04.002 Bibcode: 2016NewA...48...49Z

Guo, Juan; Zhang, Ling; Yin, Jian-qin +2 more

We present an automatic algorithm to detect coronal mass ejections (CMEs) in Large Angle Spectrometric Coronagraph (LASCO) C2 running difference images. The algorithm includes 3 steps: (1) split the running difference images into blocks according to slice size and analyze the grayscale statistics of the blocks from a set of images with and without…

2016 New Astronomy
SOHO 6
V421 Pegasi: a detached eclipsing binary with a possible γ Doradus component
DOI: 10.1016/j.newast.2015.12.004 Bibcode: 2016NewA...46...47O

Akan, C.; Çakırlı, Ö.; Özdarcan, O.

We present spectroscopic and photometric study of V421 Peg. This eclipsing binary displays lines from both components that are well separated. This allowed us to classify the primary and secondary component as F(1 ± 0.5) V and F(2 ± 0.5) V, respectively. We use our radial velocity measurements together with Hipparcos and ASAS photometry and apply …

2016 New Astronomy
Hipparcos 3
Abundance analysis of the supergiant stars HD 80057 and HD 80404 based on their UVES Spectra
DOI: 10.1016/j.newast.2016.02.006 Bibcode: 2016NewA...47...46T

Baştürk, Ö.; Tanrıverdi, T.

This study presents elemental abundances of the early A-type supergiant HD 80057 and the late A-type supergiant HD 80404. High resolution and high signal-to-noise ratio spectra published by the UVES Paranal Observatory Project (Bagnulo et al., 2003) were analyzed to compute their elemental abundances using ATLAS9 (Kurucz, 1993; 2005; Sbordone et a…

2016 New Astronomy
IUE 3
First analysis of eight Algol-type binaries: EI Aur, XY Dra, BP Dra, DD Her, VX Lac, WX Lib, RZ Lyn, and TY Tri
DOI: 10.1016/j.newast.2015.06.009 Bibcode: 2016NewA...42....1Z

Zasche, P.

The available photometry from the online databases were used for the first light curve analysis of eight eclipsing binary systems EI Aur, XY Dra, BP Dra, DD Her, VX Lac, WX Lib, RZ Lyn, and TY Tri. All these stars are of Algol-type, having the detached components and the orbital periods from 0.92 to 6.8 days. For the systems EI Aur and BP Dra the …

2016 New Astronomy
INTEGRAL 1