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J/ApJ/834/196    Galactic novae with m≤10 from 1900 to 2015    (Shafter, 2017)

The Galactic nova rate revisited. Shafter A.W. <Astrophys. J., 834, 196-196 (2017)> =2017ApJ...834..196S (SIMBAD/NED BibCode)
ADC_Keywords: Novae ; Magnitudes ; Milky Way Keywords: Galaxy: stellar content; novae, cataclysmic variables; stars: statistics Abstract: Despite its fundamental importance, a reliable estimate of the Galactic nova rate has remained elusive. Here, the overall Galactic nova rate is estimated by extrapolating the observed rate for novae reaching m≤2 to include the entire Galaxy using a two component disk plus bulge model for the distribution of stars in the Milky Way. The present analysis improves on previous work by considering important corrections for incompleteness in the observed rate of bright novae and by employing a Monte Carlo analysis to better estimate the uncertainty in the derived nova rates. Several models are considered to account for differences in the assumed properties of bulge and disk nova populations and in the absolute magnitude distribution. The simplest models, which assume uniform properties between bulge and disk novae, predict Galactic nova rates of ∼50 to in excess of 100 per year, depending on the assumed incompleteness at bright magnitudes. Models where the disk novae are assumed to be more luminous than bulge novae are explored, and predict nova rates up to 30% lower, in the range of ∼35 to ∼75 per year. An average of the most plausible models yields a rate of 50-23+31yr-1, which is arguably the best estimate currently available for the nova rate in the Galaxy. Virtually all models produce rates that represent significant increases over recent estimates, and bring the Galactic nova rate into better agreement with that expected based on comparison with the latest results from extragalactic surveys. Description: In this paper, we reconsider the analysis presented in Shafter (2002AIPC..637..462S) and Shafter (1997ApJ...487..226S) by conducting Monte Carlo simulations to estimate the global Galactic nova rate and its uncertainty. The revised analysis includes the increased sample of Galactic novae available since 2000. From 1900 to the end of 2015 there have been a total of ∼250 Galactic novae discovered brighter than m=10, and we have compiled a list of these novae in Table 1. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 53 256 Galactic novae since 1900
See also: II/173 : A REFERENCE CATALOGUE OF GALACTIC NOVAE (Version 1990.0) J/ApJS/227/1 : HST survey for novae in M87. I. VI LCs (Shara+, 2016) J/A+A/580/A45 : Nova M31N 2008-12a 2014 eruption in optical/UV (Darnley+, 2015) J/ApJS/219/26 : OGLE atlas of classical novae. I. Galactic bulge (Mroz+, 2015) J/ApJ/788/164 : Properties of known Galactic classical novae (Pagnotta+, 2014) J/A+A/554/A123 : Near-IR catalog of novae in VVV survey area (Saito+, 2013) J/ApJS/187/275 : Photometric histories of recurrent novae (Schaefer, 2010) J/PAZh/34/278 : Distances and extinction of Galactic novae (Burlak, 2008) J/PAZh/34/270 : Photometric parameters of Galactic novae (Burlak+, 2008) J/other/NewA/13.133 : 2MASS photometry of cataclysmic variables (Ak+, 2008) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 13 A13 --- Nova Nova identifier 15- 23 A9 --- Name IAU identifier 25- 34 A10 "Y/M/D" Date UT date of maximum light 36- 40 F5.1 deg GLON Galactic longitude 42- 46 F5.1 deg GLAT Galactic latitude 48- 51 F4.1 mag mag [-1.1/10] Magnitude at maximum (1) 53 I1 --- Ref Reference (2)
Note (1): Peak magnitude when available, otherwise discovery magnitude. Note (2): Reference as follows: 1 = http://asd.gsfc.nasa.gov/Koji.Mukai/novae/novae.html 2 = http://www.cbat.eps.harvard.edu/nova_list.html 3 = http://projectpluto.com/galnovae/galnovae.htm 4 = Schaefer 2010, J/ApJS/187/275
History: From electronic version of the journal
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 31-Jul-2017
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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