AHubble Space TelescopeSurvey for Novae in M87. II. Snuffing out the Maximum Magnitude–Rate of Decline Relation for Novae as a Non-standard Candle, and a Prediction of the Existence of Ultrafast Novae-Reference-Cited by-同舟云学术

AHubble Space TelescopeSurvey for Novae in M87. II. Snuffing out the Maximum Magnitude–Rate of Decline Relation for Novae as a Non-standard Candle, and a Prediction of the Existence of Ultrafast Novae

Published:2017-04-21 Issue:2 Volume:839 Page:109
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Shara Michael M.^ORCID,Doyle Trisha,Lauer Tod R.^ORCID,Zurek David,Baltz Edward A.,Kovetz Attay,Madrid Juan P.,Mikołajewska Joanna^ORCID,Neill J. D.^ORCID,Prialnik Dina,Welch D. L.^ORCID,Yaron Ofer

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/839/i=2/a=109/pdf

Reference55 articles.

1. Novae in the Andromeda nebula.

2. The Resolution of Messier 32, NGC 205, and the Central Region of the Andromeda Nebula.

3. The inner halo of M 87: a first direct view of the red-giant population

4. Distance of the Large Magellanic Cloud through the maximum magnitude versus rate of decline relation for novae

5. Properties of the nova population in M31

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