Properties of the nova population in M31-Reference-Cited by-同舟云学术

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Properties of the nova population in M31

Published:1989-06 Issue: Volume:97 Page:1622
ISSN:0004-6256
Container-title:The Astronomical Journal
language:
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Author:

Capaccioli Massimo,della Valle Massimo,Rosino Leonida,D'Onofrio Mauro

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 156 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Exploring the Maximum Magnitude versus Rate of Decline Relation for Novae in M31;The Astrophysical Journal Supplement Series;2024-05-17

2. The size–mass and other structural parameter (n, μz, Rz) relations for local bulges/spheroids from multicomponent decompositions;Monthly Notices of the Royal Astronomical Society;2022-12-19

3. Ram pressure stripping and ISM disc truncation: prediction versus observation;Monthly Notices of the Royal Astronomical Society;2022-10-04

4. The Galactic Nova Rate: Estimates from the ASAS-SN and Gaia Surveys;The Astrophysical Journal;2022-09-29

5. The Rate and Spatial Distribution of Novae in M31 as Determined by a 20 Year Survey;The Astrophysical Journal;2022-09-01

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