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ArticlePeer ReviewedOpen AccessPlagiarism Passed
Paper ID:10.55041/IJSREM38554

NGC 6826- Integrated Study of the Planetary Nebula and Central Star Properties

Stream/Area:

-

Subject:

-

Paper ID:

10.55041/IJSREM38554

Volume:

8 |

11 |

Nov 2024

Pages:

Publication Frequency:

Monthly (12 issues per year)

DOI
Digital Object Identifier
10.55041/IJSREM38554

License:International Journal of Scientific Research in Engineering and Management follows the Creative Commons Attribution 4.0 (CC BY 4.0) License, allowing free use and distribution with proper attribution.

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Authors

RR

Rajesh Rajaan

LK

Loveleen Kumar

NC

Nilam Choudhary

AS

Aakriti Sharma

HSG

Harpreet Singh Gill

KS

Kailash Soni

MB

Mani Butwall

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Abstract

This study provides a comprehensive analysis of NGC 6826, focusing on the structural, kinematic, and spectroscopic properties of its planetary nebula and the characteristics of its central star. By integrating multi-wavelength observational data, we examine the nebular morphology, ionization structure, and chemical composition, which reveal insights into the evolutionary processes shaping the nebula. Additionally, we analyze the central star’s luminosity, temperature, and spectral features to understand its role in driving the observed nebular dynamics. Our findings contribute to the broader understanding of planetary nebula formation, central star evolution, and the interaction mechanisms at play. This integrated approach underscores the importance of studying planetary nebulae in a holistic context to unravel the complexities of stellar evolution.

KEYWORDS

NGC 6826 planetary nebula central star kinematics stellar evolution spectroscopy

Cite This Article

Rajesh Rajaan, Loveleen Kumar, Nilam Choudhary, Aakriti Sharma, Harpreet Singh Gill, Kailash Soni, Mani Butwall, "NGC 6826- Integrated Study of the Planetary Nebula and Central Star Properties," International Journal of Scientific Research in Engineering and Management, vol. 8, no. 11, Nov 2024. https://doi.org/10.55041/IJSREM38554

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Publication Date

11/10/2024

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Double-Blind Peer Review

Review Rounds: 2

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